The galaxy presents an elliptical morphology, with a smooth light distribution characterized by a high degree of central concentration. The galaxy exhibits a slightly elongated shape, appearing more "in between" oval than perfectly round or cigar-shaped. There is subtle evidence of morphological disturbance in the galactic structure, possibly indicating a past or ongoing interaction with another galaxy. Star formation activity appears suppressed with little to no indication of distinct spiral arms or HII regions. It is situated at a moderate redshift suggesting a substantial distance. The overall color profile implies a population of older stars.
