The galaxy presents a predominantly smooth, elliptical morphology. There is a bright, concentrated central bulge that appears yellowish in color. This suggests an older stellar population is dominant in the core. Extending outwards from the core is a more diffuse halo, which exhibits a subtle flattening and a slight cigar shape. The halo shows hints of bluer colors, particularly towards the periphery, possibly indicating some regions of recent or ongoing star formation. There are no apparent signs of major disturbances, tidal tails, or merging activity in the image. Faint spiral arms or disk features are not readily discernible, and the galaxy seems to lack prominent dust lanes. The overall structure points to a galaxy with a relatively relaxed morphology, potentially consistent with an early-type classification.
