The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a moderate elongation. The core is characterized by a strong concentration of light, appearing significantly brighter and more yellow in color. The light decreases gradually outwards from the center. Faint, diffuse extensions are slightly visible beyond the concentrated core, though they are less defined. There are no distinct spiral arms or prominent dust lanes visible. Overall, the galaxy's morphology suggests a system dominated by an older stellar population, with little evidence of ongoing or recent major star formation. There is no obvious evidence of tidal disturbances or ongoing mergers.
