The galaxy presents as a relatively smooth, elliptical-like object. It exhibits a generally rounded morphology, though perhaps slightly elongated. The central region appears bright and concentrated, suggestive of an older stellar population. The overall color profile is redder, indicating a lack of significant ongoing star formation. There may be some minor disturbances or interactions visible, though the dominant impression is that of a relatively relaxed, evolved system. Further investigation into its velocity dispersion and stellar populations would be beneficial.
