The galaxy presents a generally smooth appearance, indicative of an elliptical or lenticular morphology. The light distribution appears centrally concentrated, with a gradual decrease in intensity towards the outer regions. While there is a slight elongation, the galaxy is mostly round in shape. There is no apparent spiral structure or evidence of recent major merger activity. Subtle color variations are present, with a yellowish hue dominating the central region and possibly bluer tints in the fainter outer disk. These colors suggest a stellar population dominated by older stars, possibly with some ongoing star formation in the outer parts of the galaxy. There are no apparent dust lanes or other signs of significant obscuration. Overall, the galaxy seems to be an evolved system, but further investigation would be needed to confirm its precise classification and properties.
