The galaxy presents a predominantly smooth morphology, appearing elliptical in shape with an approximate ratio of 3:1 for major to minor axis. The core exhibits a concentrated luminosity profile, suggesting a high stellar density in the central region. The color gradient indicates a population of older stars, with the central bulge displaying a yellowish-orange hue while the outer regions show a slight hint of blue. There is no apparent spiral structure or significant dust lane visible. The galaxy appears relatively isolated, with no obvious signs of interaction or merging events.
