The galaxy presents a generally smooth, elliptical morphology. The light profile appears highly concentrated towards the center, suggesting a prominent bulge. A secondary, less defined light concentration is visible on one side of the main body. The color gradient indicates a redder central region transitioning to slightly bluer tones towards the outer edges, possibly indicating older stellar populations in the core and regions of more recent star formation further out. There are possible interactions occurring, visible as a potential merger. The system appears relatively undisturbed overall, but the galaxy shows a complex light distribution. Based on the observed features, this galaxy can be described as a relatively massive system with a moderate amount of ongoing star formation.
