The galaxy presents as a diffuse, elongated object with a somewhat smooth appearance. Its morphology suggests a possible elliptical or lenticular classification, though a highly inclined spiral cannot be ruled out with this image resolution. There is a slight variation in color across the galaxy's body; the central region appears somewhat redder compared to the bluer outer edges.

Evidence for significant ongoing star formation within the galaxy is not apparent from visual inspection alone. The galaxy does not appear to be undergoing a major merger, although there is a possible minor disturbance detected, potentially indicating an interaction with a smaller companion galaxy that might have occurred sometime in the past.
