The galaxy appears to be a relatively compact and smooth object. The light profile suggests a concentrated central bulge or core, with a gradual decrease in luminosity outward. It exhibits a roughly circular or elliptical morphology; its shape is quite regular. There is no readily apparent spiral structure or obvious disk-like component. The galaxy exhibits a yellowish hue toward the center, potentially indicating an older stellar population. The lack of prominent blue light suggests minimal active star formation. There is no evidence of tidal tails, bridges, or other features suggestive of recent major merger activity. The galaxy is fairly isolated, lacking any immediately apparent companion galaxies or interacting structures. There are no clear signs of significant dust lanes or patchy obscuration within the galaxy.
