The galaxy presents as a somewhat elongated, elliptical structure. Its central region appears to be dominated by older stellar populations, indicated by the reddish-orange hue. Moving outward from the core, the color transitions slightly toward a bluer tone, suggesting the presence of younger, hotter stars in the outer regions. This color gradient could be indicative of ongoing, albeit modest, star formation activity. There is a general smoothness to the galaxy's light distribution, implying that it is likely a relatively undisturbed system. Overall, the galaxy exhibits a morphology consistent with an early-type spiral or elliptical galaxy, with a likely mass within the range of a large galaxy.
