The galaxy presents as a relatively smooth, centrally concentrated object. The light distribution suggests an elliptical morphology, with minimal evidence of spiral arm structure or a prominent disk component. The central region exhibits a yellowish hue, possibly indicative of an older stellar population. Fainter, blue-ish halos extend outward from the central core, possibly showing some ongoing star formation. No signs of significant tidal disturbances or major mergers are readily apparent, though a faint object seems to lie near the main object, and may be an indication of minor disturbance. Overall, the galaxy appears to be an early-type system, potentially a massive elliptical galaxy, located at a moderate cosmological distance.
