The galaxy presents as a slightly elongated spheroid with a smooth, centrally concentrated light profile. There is a prominent bulge exhibiting high luminosity, with the light intensity gradually decreasing towards the outer regions. Hints of a disk component are visible in the form of a flattened structure, though features indicating spiral arms or bar structures are not readily apparent. The galaxy displays a generally uniform color, suggesting a relatively homogenous stellar population across its entirety, although a slight color gradient might be present. There is not a lot of dust present, but there is some in the dimmer outer regions. Overall, the galaxy exhibits features consistent with an elliptical galaxy or possibly an early-type spiral galaxy viewed at an oblique angle. There is the indication of minor disturbances, which may be the result of a possible minor merger. 
