The galaxy exhibits a generally elliptical morphology, appearing mostly smooth with a concentrated central bulge. There is a slight flattening of the overall shape, but the galaxy does not present a pronounced disk structure. The central region appears brighter and exhibits a yellowish hue, potentially indicating an older stellar population. Fainter, diffuse blue light can be seen extending from the core, which could represent ongoing star formation. There is no obvious strong spiral structure or any significant tidal disturbances to the galaxy. The color gradient suggests the galaxy is not undergoing a major merger.
