The galaxy presents as a centrally concentrated system, appearing largely smooth in morphology. Its overall shape tends towards circular, with a slight hint of ellipticity that is barely detectable. There is a bright, somewhat diffuse nucleus. Moving outward from the core, the luminosity gradually decreases, with the outer regions exhibiting fainter and bluer hues. No distinct spiral arm structure or prominent dust lanes are visible. The galaxy appears relatively undisturbed, showing no signs of major tidal interactions or ongoing merging events. Subtle irregularities are visible in the halo, with minor suggestions of past accretion events. The estimated size indicates that this is a relatively large galaxy, although there appears to be relatively little star formation. The color indices suggest it hosts a significant population of older stars, though there appears to be a small amount of on-going star formation.
