The galaxy presents as a relatively smooth, elliptical structure. It has a bright, concentrated core that transitions smoothly into a more diffuse halo. The color profile suggests a population of older stars, exhibiting a yellowish-red hue. There appears to be a lack of distinct spiral arm structure or significant dust lanes. The galaxy appears to be somewhat round in shape, with a minor deviation towards an elongated, cigar-like form. There are no obvious signs of ongoing mergers or significant tidal disturbances in the image. Overall, the galaxy morphology points toward an evolved system with suppressed star formation.
