The galaxy appears as a single, luminous object with a relatively smooth morphology. It exhibits a concentrated central region, likely a galactic bulge, that gradually fades outwards into a diffuse halo. There's a slight elongation in the observed structure but it generally appears elliptical or spheroidal, rather than a well-defined spiral disk. No distinct spiral arms or prominent dust lanes are evident. The galaxy's color profile suggests a relatively older stellar population as the light is more concentrated in the redder wavelengths. The galaxy does not appear to be strongly interacting or undergoing a major merging event.
