The galaxy presents an elongated, cigar-shaped morphology, with a relatively smooth appearance. The central bulge exhibits a reddish hue, potentially indicating an older stellar population and a lower rate of star formation in this region. Surrounding the bulge is a disk component displaying a greenish tint, suggesting the presence of younger stars or ionized gas. This implies ongoing, but perhaps subdued, star formation activity in the disk. The galaxy appears relatively undisturbed, without any major signs of merging or tidal interactions. There may be a small companion on the left of the image. The overall color profile suggests a transition from a predominantly older, quiescent population in the central regions to a younger, star-forming population within the galactic disk.
