The galaxy presents as a relatively smooth, centralized structure with a bright core, suggestive of a significant bulge component. The overall shape is somewhat elliptical, appearing mostly rounded with a slight elongation. There is no obvious spiral arm structure or bar visible. Faint extensions emanate from the central region, gradually fading into the background. No major disturbances or signs of ongoing merger activity are discernible. The light distribution appears dominated by older stellar populations, reflected in the yellowish hue, indicating a comparatively low rate of current star formation. There are no pronounced dust lanes or prominent star-forming regions visible.
