The galaxy presents an elongated, cigar-like morphology. It exhibits a smooth, diffuse light distribution, suggesting a relatively uniform stellar population. There is a slight color gradient, with the central region appearing more yellowish and the outer regions trending towards a bluer hue. This could indicate a higher concentration of older stars in the galactic nucleus and younger, hotter stars in the outer regions. The galaxy appears relatively undisturbed, showing no signs of major mergers or significant tidal interactions. However, there may be a minor disturbance present, based on the slight asymmetry in its shape. Overall, the galaxy appears to be a relatively massive system, with moderate star formation activity.
