The galaxy presents as a fairly compact object with a smooth, elliptical morphology. There is no evidence of strong spiral arm structure or a prominent central bar. The color profile indicates a redder population, consistent with a higher concentration of older stars and potentially less ongoing star formation. The light distribution appears relatively uniform, without significant bright knots of star formation or irregular features suggestive of recent mergers or tidal interactions. The galaxy is moderately luminous. A slight elongation is observable, though the overall shape remains largely spheroidal.
