The galaxy presents as a centrally concentrated elliptical morphology. The light profile appears smooth with no discernible spiral arm structure or significant dust lanes. The color gradient suggests an older stellar population, with a reddish-yellow hue dominating the core region. There is a slight elongation observed, but overall the galaxy is moderately round. Faint, diffuse extensions may be present, indicating possible tidal features or past interactions, although these are not prominent. The galaxy appears relatively isolated with no obvious signs of a major ongoing merger or significant disruption.
