The galaxy presents as a luminous object with a generally smooth morphology. It appears to be elliptical or lenticular in shape, lacking any obvious spiral arm structures. The central region exhibits a higher concentration of luminosity, suggesting a prominent galactic nucleus. The color profile indicates a relatively older stellar population, appearing more yellow/orange, suggestive of reduced ongoing star formation. There is a possibility of minor disturbance or interaction indicated by a slight asymmetry or distortion in the overall shape, but it primarily presents as a relatively undisturbed system.
