The galaxy presents as a generally smooth, elliptical or lenticular structure. Its color profile indicates a dominant population of older stars, inferred from the redder hues concentrated in the central region. This suggests that star formation is likely suppressed or has occurred at a low rate in the recent past. The galaxy lacks prominent spiral arms or any clear indication of active galactic nuclei (AGN) activity in the form of bright, compact emission. There appears to be no significant ongoing interaction or merging events with other galaxies in the immediate vicinity, based on the lack of tidal tails or other obvious morphological disturbances. Its apparent roundness is observed with no cigar-shaped features. Overall, the galaxy appears to be a relatively quiescent, evolved system.
