This galaxy presents as a lenticular or possibly an elliptical galaxy, elongated in shape, with a smooth, centralized light distribution. A prominent bulge dominates the core, exhibiting a yellowish-orange hue, suggesting an older stellar population. A fainter, bluer disk is faintly visible at the upper left region of the galaxy, indicating the presence of some younger stars and potentially ongoing, though low-level, star formation in at least one region. There's no clear evidence of strong spiral arms, and the galaxy appears generally undisturbed, showing no major morphological distortions indicative of recent major mergers. The overall color gradient indicates a progression from older stars in the core to younger populations in the outer regions, though this difference is very subtle.
