The galaxy appears as a centrally concentrated object with a generally smooth morphology. There is little evidence of spiral arm structure or distinct features such as dust lanes. The light profile suggests a primarily spheroidal shape, with a gradual decrease in luminosity from the core outwards. The core region displays a yellowish hue, potentially indicating a population of older stars and relatively low levels of ongoing star formation. The overall color suggests a relatively evolved stellar population. There is very faint surrounding light that fades into the background. There is no obvious sign of any major mergers or tidal disturbances. The object appears to be generally undisturbed.
