The galaxy presents as a centrally concentrated object, exhibiting a smooth, largely featureless morphology. The central region displays a distinct yellowish hue, suggestive of an older stellar population. A gradual decline in luminosity is observed moving outward from the core, transitioning into a faint, diffuse halo. The overall shape appears elliptical or spheroidal, with no discernible spiral arm structure or prominent dust lanes. There are slight color variations in the outer regions of the galaxy, likely due to differing stellar populations. No strong evidence of ongoing merger activity or major disturbances is immediately apparent in the image. The galaxy's profile suggests a lack of significant recent star formation activity.
