This galaxy presents a moderately bright, elliptical morphology. It appears to be relatively smooth in texture, lacking prominent spiral arms or distinct dust lanes. The central region exhibits a high degree of luminosity, suggesting a concentrated stellar population or an active galactic nucleus.

The overall color profile suggests a population of older stars, exhibiting a yellowish-red hue. There is subtle evidence of some bluer regions scattered throughout the galaxy, possibly indicating localized regions of recent star formation. Based on the morphological characteristics, this galaxy is likely an elliptical or lenticular type, exhibiting properties consistent with a post-starburst system. The size of the galaxy is moderately large, implying a substantial mass. There are some hints of minor disturbance within the galaxy, possibly signs of tidal interactions or small mergers.
