The galaxy presents as a relatively compact object with a somewhat smooth appearance. Its shape is broadly elliptical, with a suggestion of slight elongation but without any obvious spiral arm structures. There is a noticeable concentration of light towards the center, indicative of a bulge. The galaxy exhibits a redder hue overall, suggesting an older stellar population or significant dust obscuration. Subtle color variations are present across the galaxy's extent, with a slightly bluer region potentially indicative of younger stars. No strong signs of a major ongoing merger or tidal disruption are readily apparent, but a minor disturbance is not ruled out.
