The galaxy presents a generally smooth and rounded morphology. The light distribution appears centrally concentrated, with a relatively rapid decrease in intensity moving outward from the core. There's no strong evidence of spiral arm structures or a well-defined disk. The object possesses a slight yellowish hue, suggesting a stellar population dominated by older stars. The overall appearance indicates that this galaxy is likely an elliptical or lenticular type, with little ongoing star formation. A very subtle irregularity can be observed which could suggest some kind of minor merger in the past.
