The galaxy exhibits a generally smooth, elliptical morphology. Its shape is elongated but not excessively so, appearing somewhere between round and cigar-shaped. There is a central concentration of light, likely indicative of a galactic bulge. This core region displays a reddish hue, potentially suggesting an older stellar population. The surrounding halo of the galaxy is less concentrated and appears bluer, possibly due to the presence of younger, hotter stars or ongoing star formation activity. There is no obvious evidence of spiral arms or a distinct disk structure. No significant merger events or major disturbances can be discerned in the visual data. Overall, the galaxy appears to be an early-type galaxy.
