The galaxy appears to be a relatively smooth, centrally concentrated object. It exhibits a generally elliptical morphology, showing a slight deviation from perfect roundness. There is a gradual decline in surface brightness from the core outwards, with no obvious spiral arm structure visible in this image. The color profile suggests a population of older stars, with a redder hue dominating the central regions. There is no indication of significant dust lanes or prominent star-forming regions. The galaxy appears relatively undisturbed, without major signs of mergers or tidal interactions.
