The galaxy exhibits a primarily elliptical morphology, appearing cigar-shaped with a high degree of elongation. The light distribution appears relatively smooth and centrally concentrated, with a gradual decrease in surface brightness towards the edges. The color profile suggests a redder core transitioning to a bluer halo. This color gradient is indicative of a stellar population gradient, with older, redder stars dominating the central region, and younger, bluer stars potentially present in the outer regions. There is no apparent spiral structure, ring structure, or strong dust lane. No signs of active galactic nuclei are apparent. Overall, the galaxy presents itself as a relatively isolated system without any obvious signs of major interaction or merging activity. The galaxy is likely at an intermediate redshift, based on the color and apparent size.
