The galaxy presents a predominantly smooth morphology, but with some visible features. A central, bright region is evident, suggesting a concentration of stars or potentially an active galactic nucleus. There appears to be a slight elongation or extension to one side of the central region, indicating a possible disk-like structure or tidal disturbance. The color profile suggests a relatively evolved stellar population, leaning towards redder hues overall, although a small amount of bluer light is detected, indicating some star formation. There seems to be an ongoing or past merging event happening in this galaxy, most likely.
