The galaxy presents a generally smooth, elliptical morphology with a concentrated central bulge. It appears moderately rounded, lacking any distinct spiral arm structures or bar features. The light profile suggests a centrally concentrated brightness distribution, indicative of an older stellar population. The color is generally redder, especially towards the core, which may be indicative of reduced recent star formation in the central regions. There are no significant signs of ongoing major mergers or tidal disturbances, and the galaxy appears relatively isolated and undisturbed. Faint, diffuse light extends beyond the central region indicating the galaxy is of considerable size.