The galaxy presents a somewhat smooth, elliptical morphology. Its color appears to be primarily reddish, suggestive of an older stellar population with lower rates of ongoing star formation, and a higher concentration of redder stars. The galaxy exhibits a moderate degree of central concentration, with the light gradually fading towards the outer regions. There is no discernible spiral arm structure or prominent dust lanes visible within the galaxy’s disk. A slight elongation is observed, but it deviates only modestly from a circular shape. No apparent signs of major mergers or significant tidal disturbances are observed in the morphology.