The galaxy presents as a luminous, roughly elliptical object. Its core exhibits a higher concentration of light, gradually decreasing outwards, suggesting a centrally concentrated stellar population. The overall color appears to be yellowish-orange, indicating a population dominated by older stars and a relatively low rate of on-going star formation. No distinct spiral arm structures or dust lanes are discernible in the image. There is a slight asymmetry in the outer regions, although its nature cannot be clearly determined. This could be the result of tidal interactions or a minor internal disturbance. The smooth and round appearance implies that it is likely an elliptical galaxy.
