The galaxy appears as a concentrated, centrally brightened object with a smooth morphology. Its overall color is yellowish-orange, suggesting a dominant population of older stars. The shape is roughly elliptical with a slight elongation, somewhere between round and cigar-shaped, lacking any discernible spiral arm structure or significant dust lanes. There is no obvious evidence of recent or ongoing major merger activity, though subtle irregularities might suggest minor gravitational interactions. The luminosity profile increases sharply towards the center, indicating a significant bulge component. The galaxy does not display prominent features typically associated with active galactic nuclei, such as bright jets or extended emission regions. The compact nature and color imply a relatively quiescent galaxy, potentially an elliptical or S0 type.
