The galaxy presents as a smooth, elongated structure. Its light is concentrated toward the center, indicating a prominent bulge. The galaxy exhibits a color gradient, with a yellowish-white central region transitioning to a redder hue at the outer edges. The shape appears to be a flattened spheroid, suggestive of an elliptical morphology. The overall form suggests an older stellar population, with minimal evidence of ongoing star formation. The disk is prominent but not necessarily spiraled. There is no evidence of recent interactions or major disturbances to its structure.
