The galaxy presents as a somewhat elliptical structure with a concentrated central bulge. The light profile appears relatively smooth, suggesting a lack of significant spiral arm structure or prominent dust lanes. The core exhibits a bright, concentrated luminosity, potentially indicative of an active galactic nucleus or a dense stellar population. The outer regions of the galaxy fade gradually into the background sky, showing a decreasing stellar density with radial distance. The color distribution is somewhat homogenous, but subtle variations imply differing stellar populations or dust content across the galaxy's extent. There is some indication of a slight tidal disturbance, as the structure appears asymmetrical and there is some extension on one side. Overall, the galaxy appears as an intermediate-stage elliptical galaxy with potential signs of past or ongoing interaction.
