The galaxy presents as an approximately elliptical structure with a bright, concentrated central region. Surrounding the central bulge, there is a discernable disk-like structure. This disk appears moderately inclined relative to our line of sight. The colour distribution across the galaxy suggests some heterogeneity in stellar populations. The central region has a pronounced blue-white hue, which might be indicative of recent or ongoing star formation or an active galactic nucleus. The outer disk displays a more complex colour pattern with hints of redder regions, potentially indicating areas dominated by older stellar populations or dust obscuration.

There appear to be some subtle irregularities in the outer disk, which could be signs of tidal interactions or past merger events. Faint extended features hint at minor disturbances, suggesting a possible interaction history.
