The galaxy presents a smooth, elliptical morphology. It exhibits a relatively high degree of ellipticity, appearing cigar-shaped. The light profile suggests a concentrated central bulge that gradually fades into the outer regions. The primary color is a yellow-white hue, which implies an older stellar population, with a small fraction of bluer light near the edges, potentially signifying some recent star formation. No distinct spiral arms or prominent dust lanes are visible. There is no indication of any major merger events or significant tidal disturbances from surrounding galaxies. Overall, the galaxy appears to be a relatively isolated, evolved system.
