The galaxy appears to be an elongated, cigar-shaped system with a smooth, centralized light distribution. The core presents a bright, concentrated region, suggestive of an older stellar population. The overall color is slightly redder than typical spiral galaxies, indicating potentially suppressed star formation activity. There is a slight blue tint to the light on the outer edges of the galaxy. There is no clear evidence of spiral arms or prominent dust lanes. Overall, the galaxy appears relatively undisturbed, without any obvious signs of recent major merger events, although there may be minor disturbances to the morphology. A faint red feature can be observed to the lower left of the main galaxy body. This may be a star forming region within the galaxy or a small merging galaxy. The size of the system is relatively compact.
