The galaxy presents as a generally smooth and rounded structure with a central bulge that exhibits high luminosity. The overall color profile appears to be redder, suggesting an older stellar population with lower ongoing star formation. The observed morphology suggests a classification leaning towards an elliptical galaxy, potentially of type E4-E5 based on the apparent ellipticity. There may be some minor asymmetry present in the extended halo, possibly indicating a past minor merger or tidal interaction, but the galaxy does not show any obvious major disturbances or merging activity.