The galaxy presents an elongated, somewhat cigar-shaped morphology. Its central region exhibits a bright, concentrated luminosity, appearing smooth and largely featureless. Moving outward from the core, the light appears to fade and there's evidence of a disk-like structure extending along the major axis. The color gradient suggests older stellar populations dominate the central bulge, while the disk component shows a bluer hue, hinting at the presence of younger, star-forming regions. There are no prominent spiral arms or significant dust lanes visible. The galaxy appears relatively isolated, with no clear signs of a major merger event or tidal disruption. The overall structure suggests it is likely an elliptical or lenticular galaxy, possibly in a transitional phase.
