This galaxy presents an elongated, cigar-shaped morphology. The central region exhibits a concentrated, bright core, suggesting a significant stellar population and/or active galactic nucleus. There is a relatively smooth transition in luminosity from the core outwards, with a slight fading towards the edges of the galactic disk.

Faint bluish hints are visible in the outer regions of the disk, implying the potential presence of younger, hotter stars and ongoing star formation. The overall structure appears relatively undisturbed, with no obvious signs of major mergers or tidal disruptions. The galaxy appears as a relatively isolated object.
