The galaxy appears to be a relatively small, cigar-shaped object, likely a lenticular or early-type spiral galaxy seen edge-on. It exhibits a smooth, diffuse light distribution with minimal signs of distinct spiral arms or prominent dust lanes. A slight color gradient is present, with a hint of bluer tones towards the outer edges and a redder hue towards the central bulge, suggesting some ongoing, albeit low, levels of star formation occurring in the disk. There is no evidence of a recent major merger event, though the slightly irregular shape could indicate a minor gravitational disturbance or past interaction. Overall, it looks like a moderately massive galaxy with relatively low star formation activity.
