The galaxy presents as a somewhat lenticular structure, appearing mostly smooth with minimal visible substructure. The light distribution suggests a concentration in the center, with a gradual decrease in luminosity towards the outer regions. The galaxy has an elliptical shape, appearing oblong. There is a slight blue tinge toward the outer edges that possibly suggests ongoing star formation. There is no prominent spiral arm structure or bar visible, and there does not appear to be evidence of any major mergers or tidal disturbances affecting the galaxy's overall morphology.
