The galaxy exhibits a relatively compact structure with a bright, concentrated central region. It appears to be a disk galaxy viewed at an oblique angle, displaying a flattened profile with an estimated extent of a few arcseconds. There is a slight indication of spiral arm structure, although poorly defined; it's more suggestive of patchy or irregular distributions of stellar populations. The central bulge appears prominent and intensely luminous, potentially indicative of a high concentration of older stars or an active galactic nucleus. The overall color gradient shifts from blue-ish hues in the central area, which might indicate ongoing star formation, towards redder colors peripherally. Faint asymmetries or distortions could suggest minor gravitational interactions or past merger events. The galaxy does not seem to be a clear, undisturbed spiral or elliptical galaxy, showing instead signs of possible interaction or internal disruption of morphology.
