This galaxy exhibits a generally smooth morphology, appearing elliptical in shape with a noticeable bulge. The light distribution suggests a centrally concentrated structure, with brightness decreasing gradually from the core outwards. The color profile indicates an older stellar population, exhibiting a yellow-red hue, especially concentrated in the bulge. There is a slight extension in one direction, indicating a possible tidal tail or disturbance, but it could also just be an artifact of the imaging. No distinct spiral arm structures or prominent dust lanes are visible. The galaxy appears relatively isolated, with no obvious signs of interaction with neighboring galaxies, though minor disturbances cannot be ruled out based on the asymmetrical light distribution and the elongation.
