The galaxy presents a generally smooth morphology with a bright central region suggestive of a substantial galactic nucleus or bulge. The overall shape appears elliptical, though some irregularities are visible at the edges. There may be some evidence of tidal disturbances, potentially indicating a recent or ongoing interaction with another galaxy, as subtle asymmetries are present in its outer halo. The color suggests a mixture of stellar populations, with a slight shift towards bluer colors in the periphery, possibly indicating areas of active star formation. The bulk of the light is emitted from the center of the galaxy, which indicates a high stellar density.
