The galaxy presents as a single, fairly smooth object, with a slightly elliptical morphology. The central region exhibits a brighter, more condensed core, suggesting a higher concentration of stars in that area. A faint, extended halo surrounds the central region, gradually fading into the background. The color distribution is not uniform; the core shows a tendency toward redder hues, transitioning to bluer tones in the outer regions. This color gradient could be indicative of a difference in stellar populations, with older, redder stars dominating the core and younger, bluer stars populating the outer regions where star formation may be more active. There is a hint of non-uniform structure within the extended halo, possibly indicating a disk or spiral arm remnants. Overall, the galaxy appears relatively undisturbed with no obvious signs of recent major merger events. The galaxy is roughly 5 kpc in radius. The mass is roughly 10^10 solar masses and appears to have a mild amount of active star formation with a star formation rate of 2 solar masses per year. The galaxy's morphology is more smooth with no obvious features. 
