The galaxy presents as a relatively smooth, elliptical form. The central region exhibits a bright, concentrated luminosity, suggesting a dense stellar population and/or an active galactic nucleus. A color gradient is present, with a slightly bluer hue on the outer edges, potentially indicating the presence of younger stars or ongoing star formation in the galactic disk. The shape is elongated, with a clear major and minor axis, indicating a non-spherical distribution of stars. No distinct spiral arms or significant dust lanes are visible. The galaxy appears to be relatively isolated, with no obvious signs of interaction or merger activity.
