The galaxy appears to be a relatively smooth, centrally concentrated object. Its morphology is primarily elliptical, with a slight elongation, but not quite cigar-shaped. The light distribution is relatively even across the galaxy, indicating a lack of prominent spiral arms or distinct features. There is no evidence of significant tidal disturbances or ongoing mergers. The color gradient suggests the presence of older stellar populations. The core appears to be relatively concentrated and slightly yellowish. Overall, the galaxy presents as a typical elliptical galaxy.
