The galaxy appears as an elliptical or lenticular-type, characterized by a generally smooth and centralized light distribution. The core region exhibits a bright yellowish-orange hue, suggesting a population of older, redder stars likely dominating the stellar content of the galactic center. 

Moving outwards from the core, the color transitions to a more diffuse and slightly less luminous yellowish tone. This suggests a diminishing density of older stars and potentially a subtle contribution from a younger stellar population compared to the galactic center. There is some indication of a flattened morphology, but it is difficult to see definitively, the overall structure appears relatively undisturbed. There is no evidence of significant spiral arm structure, prominent dust lanes, or recent major merger events. The light is quite red suggesting minimal star formation at the time the data was collected.
