The galaxy presents as a centrally concentrated object, exhibiting a smooth, relatively featureless morphology. Its overall shape approximates an ellipse, with a moderate degree of ellipticity but is closer to being round. A bright, yellowish central bulge dominates the galaxy's luminosity profile. Fainter, bluer extensions are observed surrounding the core, which may indicate the presence of a galactic disk or an extended halo of stars. There is no apparent evidence of strong spiral arms or significant dust lanes. The galaxy appears isolated, showing no immediate signs of tidal interactions or ongoing mergers, although a slight asymmetry hints at a possible past minor disturbance.
