The galaxy presents a largely smooth morphology with a concentrated central bulge. There is little to no evidence of spiral arm structure or distinct features within the disc, implying a relatively evolved stellar population with reduced ongoing star formation. The galaxy exhibits an elliptical to slightly disk-like shape. Its color suggests a redder spectral energy distribution, indicating a dominance of older stars. The galaxy appears to be an isolated system with no signs of major mergers or significant tidal disturbances.
