The galaxy presents as a relatively smooth, elliptical-like structure. Its overall shape is elongated, with a major axis notably longer than its minor axis, trending towards a cigar shape. The light distribution is centrally concentrated, with a bright core that gradually fades into the outer regions. A slight color gradient is perceptible, with the central region appearing more yellowish-white, possibly indicating an older stellar population. The outer regions appear somewhat bluer, which might hint at the presence of younger stars, although this is subtle. There is no readily apparent disk structure, spiral arms, or active star-forming regions. No major disturbances or signs of recent merger activity are visually detected.
