The galaxy presents a diffuse, elliptical morphology. A bright, concentrated central bulge is apparent, exhibiting a yellowish hue suggestive of an older stellar population. Surrounding the bulge is a fainter, more extended halo with a bluish tinge. The smooth distribution of light within the halo indicates a lack of prominent spiral arms or distinct features. There appears to be a small degree of asymmetry in the outer regions of the halo, possibly indicative of a minor interaction or disturbance. Overall, the galaxy appears to be relatively quiescent, showing no obvious signs of recent major mergers or intense star formation activity, but showing some signs of low activity and/or minor disturbance.
