The galaxy presents a generally smooth, elliptical morphology. Its color profile exhibits a central concentration of yellow-orange light, fading into a less intense reddish hue towards the outer regions. No distinct spiral arm structures or prominent dust lanes are discernible. The light distribution suggests a centrally condensed stellar population with a potentially older stellar population dominating the observed light. The galaxy appears relatively undisturbed, with no obvious signs of ongoing major mergers or tidal interactions affecting its overall structure, although there may be a minor disturbance. There is a general roundedness.
