The galaxy appears to be a relatively smooth, early-type galaxy, likely an elliptical or lenticular. It exhibits a concentrated central bulge that gradually fades into the outer regions. The galaxy possesses a somewhat elongated, cigar-like shape. There is little to no discernible spiral arm structure or prominent dust lanes. The color appears to be somewhat redder, suggesting an older stellar population and suppressed star formation activity. There is no evidence of significant tidal disturbances or ongoing mergers in the immediate vicinity. It appears to be an isolated galaxy with a quiescent morphology.
