The galaxy presents as an elliptical morphology, with a pronounced central bulge exhibiting a high surface brightness. The overall color appears redder in the central regions, suggestive of an older stellar population. Moving outwards, the color gradients indicate a slightly bluer halo, possibly indicating some more recent star formation activity in the outer regions or contributions from a younger stellar population. The galaxy exhibits a degree of flattening, departing from a perfectly circular shape. There is no apparent structure such as spiral arms, a bar, or obvious dust lanes visible in this image. The galaxy appears relatively isolated, showing no signs of major tidal interactions or ongoing mergers. The overall impression is that of a relatively massive galaxy, likely a lenticular or elliptical galaxy, with some signs of low-level star formation.
