The galaxy presents as a moderately luminous, elliptical morphology. It exhibits a smooth, concentrated light profile with a central bulge that appears more yellow-red, suggesting an older stellar population is centrally located. The galaxy has a somewhat elongated shape, displaying a cigar-like appearance. There appears to be minimal to no evidence of spiral arms or significant disk features, with a relatively smooth transition in color and brightness from the core to the outer regions. There is little to no noticeable dust, indicating the galaxy is gas-poor with a suppressed star formation rate. No signs of any major ongoing mergers, tidal tails, or any significant disturbances are observed.
