The galaxy appears as an elliptical or lenticular system, exhibiting a smooth, relatively featureless morphology. It presents a moderate elongation, with an axis ratio suggesting a shape somewhere between a perfect sphere and a more cigar-like form. There is no apparent indication of a strong disk component or spiral arm structure. The galaxy's color index suggests a population dominated by older stars, with only subtle variations in color across its extent. No signs of active galactic nuclei activity, major mergers, or significant tidal disturbances are readily discernible in the image. However, minor disturbances cannot be ruled out. The galaxy is moderately luminous, suggesting a substantial stellar mass.
