The galaxy appears to be a relatively smooth, centrally concentrated object. Its morphology is largely elliptical, presenting a fairly regular and well-defined shape. There is minimal evidence of spiral arm structure or significant disk features. The color profile indicates a general redder hue, suggesting an older stellar population. There are no obvious tidal tails or other features indicating recent major merger activity. The overall texture seems homogenous, showing little sign of active star formation regions or prominent dust lanes. Faint light extends outwards from the central region.
