The galaxy appears to be a relatively smooth, elliptical or lenticular galaxy with a concentrated light profile. It exhibits a nearly circular morphology, showing no discernible spiral arms or bar-like structures. The color gradient suggests a dominant population of older stars. The central region appears yellowish, indicative of aging stellar populations, with a more uniform distribution of light throughout the galaxy's body. There is little evidence of ongoing star formation. Possible minor tidal disturbances or a faint, unresolved companion galaxy cannot be entirely ruled out, but the overall structure indicates a relaxed and evolved system.
