The galaxy presents as a relatively compact object, exhibiting an overall smooth morphology. The light distribution appears concentrated, with a bright, almost stellar-like central region. This core is surrounded by a more diffuse, extended halo. The shape approximates a rounded form, though slight irregularities may be present suggesting it is between a perfectly circular shape and something more oblong. Color variation is apparent, with a bluish-white hue dominating the core and a progression toward yellowish-red tones in the outer regions, potentially indicative of varying stellar populations or dust absorption. There appears to be evidence of some tidal disturbances or minor interactions in the overall shape of the galaxy and the halo, but these features are very faint. The bulk of the galaxy is relatively concentrated and has a defined boundary. Further investigation is necessary to confirm if the galaxy is undergoing or has undergone a merging event.
