The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The color profile exhibits a yellowish-red hue, suggesting an older stellar population. There is no apparent dust lane or spiral arm structure visible. The galaxy appears to be a single, coherent object with no signs of ongoing major mergers or significant tidal disturbances. Its morphology is fairly uniform and well-defined, indicating a dynamically evolved system. There is a slight color gradient, with the central region appearing more yellow, possibly indicating a higher concentration of older stars toward the nucleus. The outer regions have a subtle red tint, although this might be due to the limitations of the imaging data at this distance. The overall appearance indicates a significant mass content.
