The galaxy presents as a somewhat elongated, elliptical structure. It exhibits a smooth morphology with a centrally concentrated bulge that appears bright and nearly unresolved. This central region fades gradually into a less dense halo. The colour of the core is a pale yellow or white, suggesting a population of older stars. Moving outward from the center, the galaxy subtly shifts towards a bluer hue in the outer regions. There are no visible spiral arms or obvious dust lanes discernible, contributing to its generally featureless appearance. The elongated shape hints at a possible classification as an elliptical galaxy of type E4 or E5 on the Hubble sequence. There is no obvious evidence of active galactic nuclei activity or signs of recent merger events. The light distribution seems relatively symmetrical, though one edge could be slightly more diffuse than the other.
