The galaxy presents as a relatively smooth, elliptical structure. The light distribution appears centrally concentrated, with a gradual decrease in intensity outwards from the core. The main body of the galaxy exhibits an elongated shape, suggesting a classification leaning towards elliptical galaxies which are more cigar-shaped. There's a subtle color gradient observed, with a slightly yellower hue towards the central region, potentially indicating an older stellar population. The outer regions appear somewhat bluer, possibly due to the presence of a younger stellar population, though this is not definitively discernible from the image alone. There is no prominent dust lane or spiral arm structure visible. No significant signs of tidal disturbances, major mergers, or interactions with other galaxies are apparent in this field of view.
