The galaxy presents as an elliptical morphology, seemingly undisturbed and without any clear signs of merging activity. A pronounced central bulge exhibits a yellowish hue, suggesting a population of older stars. Surrounding the bulge, a fainter disk is observed, exhibiting a bluer color profile that implies the presence of some ongoing star formation. The disk is relatively smooth, without any prominent spiral arm structures immediately discernable in the available resolution. The galaxy appears moderately inclined relative to our line of sight. Overall, the galaxy gives the impression of a relatively mature system, with an appreciable spheroidal component and a less pronounced star-forming disk.
