The galaxy presents a generally smooth, elliptical morphology. The core exhibits a bright, concentrated luminosity profile, suggesting a high stellar density. The luminosity gradually decreases outwards from the core, with the outer regions appearing more diffuse. The galaxy appears to be highly inclined, as evidenced by its elongated shape. No distinct spiral arm structures or prominent dust lanes are discernible. The overall color profile indicates a likely evolved stellar population, with a dominant redder hue. There is a slight asymmetry in the light distribution with a hint of a broader bulge on one side which may indicate a prior interaction or possible weak disk component.
