The galaxy presents a largely smooth, elliptical morphology. It is centrally concentrated with a bright, unresolved core, indicative of a substantial bulge component. The galaxy appears nearly circular in projection. There is no discernible evidence of spiral arms or a prominent disk. Faint, diffuse emission extends outwards from the core, gradually fading into the background. No signs of major mergers or tidal disturbances are apparent. The overall color is consistent with an older stellar population. Star formation is likely suppressed.
