The galaxy presents as a luminous, centrally concentrated object with a relatively smooth overall appearance. The core region exhibits a bright, yellowish-white hue, indicating a high density of stars, potentially an older stellar population. There is a slight elongation to the galaxy's shape, suggesting it may be transitioning from a purely elliptical morphology. A faint, diffuse halo surrounds the central bulge, fading into the background sky. There are slight hints of possible substructure or faint tidal features. Overall, it appears to be an intermediate-mass system with a moderate level of ongoing star formation. There are no obvious signs of a recent major merger, although minor disturbances cannot be ruled out. The galaxy's color suggests a mix of stellar ages, with a more prominent older population in the center.
