The galaxy presents a generally smooth morphology. There's a centrally concentrated bulge with a bright core. Extending outward, the light distribution becomes more diffuse, though lacking well-defined spiral arm structures. The overall shape is elliptical, although there might be a hint of a disk component when considering the distribution of the fainter light surrounding the central bulge. There's a possible indication of minor disturbance or interaction with a neighbor, as evidenced by a slight asymmetry in the outer regions. However, based on the image data, the galaxy appears relatively isolated and not undergoing a major merger event. The color profile suggests an older stellar population, with the core appearing more yellow/red and bluer regions being relatively faint and localized. 
