This galaxy presents an overall elliptical morphology, although with some irregularity in its outer regions. The central bulge is bright and concentrated, exhibiting a bluish-white hue, suggesting a population of younger, hotter stars and potentially ongoing star formation. Moving outward from the core, the galaxy transitions to a fainter, greenish-yellow color, implying a mix of stellar populations with a possible increase in older stars or dust obscuration. The outer edges of the galaxy appear somewhat diffuse and uneven, hinting at possible tidal interactions or disturbances in the past. While generally appearing smooth, there is a faint suggestion of a faint arm-like feature, possibly indicating some level of disk structure. The overall light distribution is relatively smooth, indicating a lack of significant star-forming regions or distinct features across the galaxy.
