The galaxy presents as a relatively smooth, elliptical or lenticular structure. It exhibits a bright, concentrated central bulge, indicative of a high stellar density, likely composed of older stars. The overall shape is elongated, leaning toward an in-between roundness. Faint disc-like features might be present, but they are not well-defined. There are no obvious signs of spiral arms. The color profile suggests the presence of both younger, bluer stars and older, redder populations within the galaxy. No prominent dust lanes or active star-forming regions are immediately apparent upon visual inspection, implying that the galaxy is likely in a later stage of its evolution, with a moderate star formation rate. There are no obvious signs of merging or tidal disturbances.
