The galaxy presents a largely elliptical morphology, exhibiting a high degree of central concentration. The core region is intensely luminous, suggesting a significant population of older stars. There is minimal visual evidence of spiral arm structure. The galaxy's overall color is yellowish-white, indicative of a relatively evolved stellar population and reduced ongoing star formation activity. Faint color variations and slight extensions are observed within the galaxy's halo, perhaps indicative of past mergers or tidal interactions, though these features are not highly pronounced. The axial ratio appears nearly circular, with a small degree of ellipticity. The light distribution suggests a smooth profile.
