The galaxy appears as a relatively compact, luminous object with a noticeable disk or feature component, though it is largely smooth in appearance. The central region exhibits a bright, concentrated core. The overall shape is inclined toward round. Faint extensions or minor disturbances could potentially be present, but the main structure appears mostly undisturbed, without signs of a major merger. There appears to be ongoing star formation, indicated by a bluer hue in parts of the galaxy.
