The galaxy presents as a single, luminous object, with a primarily smooth morphology. The central region exhibits a concentrated brightness, suggesting a prominent bulge component. There is a slight asymmetry to the overall form, possibly indicating minor disturbances or interactions. A faint, diffuse extension or tidal feature appears on one side, hinting at past or ongoing gravitational interactions. The color profile suggests an older stellar population, potentially with reduced ongoing star formation. Overall the galaxy appears to be in the later stages of its evolution.