The galaxy presents an overall smooth and somewhat rounded appearance, characteristic of an elliptical or lenticular morphology. There is a noticeable central bulge that appears bright and concentrated. The light profile gradually decreases from the center outwards, with no clear spiral arm structure or distinct features visible. A slight blue tinge is detectable around the central bulge, potentially indicating some degree of recent star formation within the outer regions. Overall, the galaxy's structure suggests a relatively evolved system with a dominant spheroid component. Evidence of any significant ongoing mergers or tidal disturbances is absent.
