The galaxy presents a generally smooth appearance. The central region exhibits a concentrated luminosity gradient, suggesting a prominent galactic nucleus or bulge. The color of the central region is distinctly yellowish-white, potentially indicating an older stellar population. The galaxy appears elliptical in shape, with an intermediate axis ratio, deviating somewhat from a perfectly circular form but lacking a pronounced elongation. There is a slight color gradient outward from the core, becoming subtly bluer towards the outer regions, possibly reflecting ongoing or recent star formation in the disk. There is no obvious evidence of tidal features, major mergers, or significant morphological disturbances in the immediate vicinity, and appears relatively isolated.
