The galaxy presents a relatively smooth, elliptical morphology, exhibiting a concentrated central bulge. Its color profile suggests an older stellar population, likely dominated by redder giants. There's a subtle color gradient from the center outwards, implying a possible decrease in metallicity or age of the stellar populations towards the outer regions. No distinct spiral arms or prominent dust lanes are discernible, corroborating the smooth characteristic. There are no obvious tidal features or signs of recent major mergers. The galaxy appears relatively undisturbed.
