The galaxy presents a generally elliptical morphology with a smooth profile. It appears to be dominated by an older stellar population, as indicated by its yellow to red color. There is little evidence of distinct spiral arm structure. The light appears to be concentrated towards the central region, which is particularly bright. Some irregularities are noticeable, potentially indicating a minor gravitational disturbance or merger event. The galaxy exhibits a moderate degree of roundness. It shows low star formation based on the observed color.
