The galaxy presents as an elliptical structure, exhibiting a smooth light distribution. The central region displays a concentrated, yellowish-orange hue, suggesting an older stellar population. Moving outwards, the galaxy gradually fades into a bluer periphery, potentially indicating the presence of younger stars. While the main body of the galaxy appears smooth, a subtle irregularity or a slight extension can be observed along its major axis. This disturbance could be indicative of a minor gravitational interaction or past merger event, though no major disturbances or tidal tails are seen. The shape of the galaxy is roughly in between round and cigar shaped, although it has an overall smooth appearance.
