The galaxy presents as a concentrated spheroid of light, approximately circular in projection. Its color profile leans towards the redder end of the spectrum, indicating a potentially older stellar population with reduced star formation activity. There is a notable lack of discernible spiral arm structures or a prominent disk. The galaxy appears relatively smooth and centrally concentrated, with a slight falloff in luminosity from the core to the outer regions. There may be a very faint, diffuse halo surrounding the main body of the galaxy, but it's difficult to distinguish this from background noise. There is no visually apparent evidence of ongoing major merging activity or tidal disturbances; however, a slight asymmetry might suggest minor interactions in its past. Overall, the galaxy's morphology suggests that it is most likely an elliptical galaxy.
