The galaxy presents as a generally smooth, elliptical form. The core region exhibits a bright, concentrated luminosity, suggesting a high density of stars. Moving outward from the core, the light intensity diminishes gradually, maintaining a relatively uniform color profile with a slight reddish-orange hue. There is minimal evidence of spiral arms or distinct substructure, instead the galaxy appears as a diffuse, somewhat rounded mass. The overall structure suggests a relatively evolved system, potentially an early-type galaxy with an older stellar population. There appears to be a minor merging event occurring.
