The galaxy presents as a relatively compact structure with a generally smooth appearance. It exhibits a dominant, centrally concentrated bulge, suggesting a classification towards the elliptical or lenticular type. There is minimal evidence of spiral arm structure or significant dust lanes. The color profile appears somewhat redder than average for galaxies at a similar redshift, hinting at an older stellar population with reduced ongoing star formation. The overall roundness is suggestive of a relaxed morphology, though there is a hint of a possible tidal interaction or recent merger event in the form of asymmetry or faint extensions. The galaxy's luminosity suggests it is a fairly massive system.
