The galaxy presents as a relatively smooth, elongated structure, consistent with a possible lenticular or early-type spiral classification. The central bulge exhibits a concentrated, bright yellowish-white luminosity, suggesting a population of older stars. Moving outwards from the core, the disk appears flattened and exhibits a color gradient, shifting towards a slightly bluer hue. This suggests the presence of younger stars, potentially accompanied by some active star formation. The galaxy appears undisturbed with no obvious signs of tidal tails or morphological distortions, which would indicate major merger events. It possesses an estimated size of ~7.6 kpc, and appears to be a massive galaxy, with moderate levels of star formation activity.
