The galaxy presents as an elongated, cigar-shaped structure with a smooth appearance. A concentration of light is observed in the central region, suggesting the presence of a galactic bulge. The light distribution indicates a relatively uniform stellar population across the galaxy, with no prominent spiral arms visible. The color is consistent with an older stellar population, with hints of ongoing star formation. Overall, the galaxy exhibits characteristics consistent with a late-type spiral or an elliptical galaxy seen edge-on. There is a hint of a minor disturbance, and could possibly be a merging event with a smaller object.
