The galaxy presents as a moderately luminous object with a somewhat spheroidal morphology. The central region appears relatively smooth and concentrated, indicating a potential bulge. Some asymmetry can be observed in the structure, possibly suggestive of a minor disturbance or interaction. A plume or tail-like structure extending from the galaxy is particularly notable, possibly caused by tidal forces. The overall color suggests the presence of evolved stellar populations. Further spectral analysis would be valuable to assess the galaxy's star formation rate and stellar population characteristics.
