The galaxy presents as a relatively smooth, elliptical morphology. A concentration of light towards the center is apparent, suggesting a high density of stars in the galactic nucleus. The color profile exhibits a broad homogeneity, with a slight shift toward redder wavelengths in the central region, possibly indicative of an older stellar population. The outer regions appear fainter and less defined, fading into the background sky. There may be faint evidence of a tidal tail or minor disturbance, but that requires further imaging to determine. Overall, the galaxy appears to be an evolved system with little evidence of active star formation.
