This galaxy appears as a relatively compact, elliptical system. The light distribution is smooth and centrally concentrated, with no discernible spiral arms or a prominent disk structure. Its shape tends to be mostly round. The galaxy exhibits a yellowish hue, suggesting a population of older stars, with a lack of significant ongoing star formation. There is no obvious sign of tidal disturbances or ongoing major mergers with other galaxies. Overall, it appears to be a relatively quiescent, evolved galaxy, likely residing at a considerable distance.
