The galaxy presents as a somewhat elliptical, unresolved object with a bright, concentrated central bulge. The core exhibits a yellowish-orange hue, suggesting an older stellar population. The outer regions of the galaxy display a gradual decrease in luminosity, fading into the background sky. There are hints of a possible disk component surrounding the bulge, though the features are subtle and lack defined spiral arms. Overall, the galaxy appears relatively smooth in texture, with no significant indications of ongoing major mergers or strong tidal disturbances.
