The galaxy presents as an elliptical structure with a smooth, centrally concentrated light distribution. The core exhibits a bright, almost unresolved, intensity. The overall color profile is predominantly blue-white, suggesting a moderate population of young, hot stars. There is a subtle hint of redder hues on one side of the galaxy which may indicate older stellar populations. The galaxy shows no obvious signs of spiral arm structure. The light profile indicates a relatively low Sersic index, typical for disk galaxies. Overall, the galaxy appears as a relatively undisturbed system, with no strong indications of recent major mergers or tidal interactions, although there is the possibility of minor disturbance.