The galaxy presents a predominantly smooth morphology, appearing elliptical in shape but with some irregularities. The central region exhibits a high concentration of light, indicating a prominent bulge. The color gradient suggests a relatively old stellar population, with the core showing a yellowish hue, potentially indicating a lack of ongoing star formation in this area. The outer regions are fainter and show some subtle extensions, perhaps tidal features or faint spiral arms that are being disrupted. There is a slight asymmetry in the overall structure, with one side appearing more extended than the other, hinting at a possible minor interaction or past merger event. The galaxy has moderate size and luminosity.
