The galaxy presents as a relatively smooth, elongated structure. Its shape is more akin to a cigar than a perfect circle. The central region exhibits a concentrated, bright luminosity, likely indicating a substantial bulge. Fainter regions of the galaxy, extending from the central bulge, indicate the presence of a galactic disk, observed nearly edge-on from our vantage point. The overall color profile indicates a possible older stellar population in the central bulge, while bluer hues in the disk hint at ongoing star formation. However, the dominance of smoother features suggests that either star formation is occurring at a low rate, or the galaxy has largely exhausted its supply of star-forming material. No signs of major mergers or significant tidal disturbances are readily apparent, although minor interactions cannot be ruled out based solely on this image.
