The galaxy presents as a relatively smooth, elliptical structure with a bright, concentrated central bulge. There is a noticeable lack of prominent spiral arms or other distinct features typically associated with disk galaxies. The core region exhibits a yellowish-white hue, suggesting an older stellar population. The galaxy fades into the surrounding space with a gradual decrease in luminosity, showing a slightly flattened shape that leans more toward being round than cigar-shaped. There appears to be no evidence of ongoing major mergers or significant tidal disturbances. Minor disturbances may be present, or they are too small to be detected in this image. Overall, the galaxy appears to be a well-formed, mature system with limited current star formation activity.
