The galaxy presents as a relatively smooth, elliptical structure with a concentrated central bulge. The light distribution is highly centralized, displaying a strong peak in surface brightness towards the core. The overall color appears to be dominated by longer wavelengths, indicative of an older stellar population, with a yellow-red hue dominating the image. There is little evidence of spiral arms or significant dust lanes. No major disturbances or tidal features can be observed, and the morphology is generally consistent with a relaxed system.
