The observed galaxy appears to be an elliptical galaxy with a smooth, centrally concentrated light distribution. The core exhibits a yellowish-orange hue, suggestive of an older stellar population. The galaxy is fairly compact and round, with a subtle extension to one side. There is no visual indication of spiral arms or prominent dust lanes. Faint outer regions surround the bright central area, gradually fading into the background. There are no obvious signs of ongoing mergers or tidal disturbances.
