The galaxy presents as a single, concentrated luminous object with a roughly elliptical morphology. The light is distributed smoothly across its surface, with no readily discernible spiral arm structure or distinct features such as star-forming regions. There is a smooth, radial falloff in light intensity from the center outwards, and a diffuse surrounding envelope. The core of the galaxy appears yellowish-white, transitioning to a redder hue in the outer regions, suggesting an older stellar population. There is no apparent evidence of a recent major merger event or significant tidal disturbances based on the smooth morphology. The object appears relatively isolated in the field.
