The galaxy presents as a relatively smooth and centrally concentrated object with a generally elliptical morphology. There is a subtle elongation visible, suggesting a deviation from a perfect circular shape, trending towards a cigar shape. The core region exhibits the highest luminosity, with a gradual decrease in intensity moving outwards. The color profile is suggestive of an older stellar population, with a general reddish hue overall, with some light blue. There is no obvious spiral arm structure or significant dust lane features visible in this image. The overall appearance implies a relatively undisturbed system, without signs of a major merger or tidal disruption.
