This galaxy presents an overall elliptical morphology, though with some notable irregularities suggesting it may be an interacting system. The primary component appears to be a relatively smooth, spheroidal structure. The core exhibits a bright, concentrated luminosity, with the light profile gradually decreasing outwards. There is some indication of a secondary component or tidal feature extending from the main body. This extension is less defined and appears more diffuse. The color distribution suggests the presence of both older stellar populations, indicated by the reddish hues, and younger, bluer stars mixed in. The galaxy has no clear dust lanes or spiral arm structure visible in this image, although some distortion in the overall shape suggests potential tidal forces or recent merger activity.
