The galaxy presents as a generally smooth, elliptical morphology. It appears largely featureless, with a concentrated central bulge and a gradually decreasing surface brightness towards its outer edges. While a spiral arm structure is not immediately apparent, there is some faint indication of a slight disc-like structure. The color profile suggests a higher concentration of older, redder stellar populations, as it appears redder in color. There is evidence of a possible minor interaction or disturbance. Overall, the galaxy is dominated by a smooth, elliptical morphology, with only subtle hints of disk features or ongoing interactions.
