The galaxy presents as a relatively bright object with a distinct elongated, cigar-like shape. It appears to possess a central bulge that is somewhat brighter and more concentrated than the surrounding galactic disk. The light distribution suggests a relatively smooth profile, though subtle variations indicate possible underlying structures. The galaxy displays a range of colors, with a slightly bluer hue dominating the outer regions and a gradient toward redder tones in the central bulge. This color gradient hints at differences in stellar populations and star formation activity across the galaxy. There's a hint of a possible minor disturbance or interaction, though no clear signs of a major merger are immediately evident. Based on its appearance, this galaxy could be classified as a late-type spiral galaxy viewed at a significant inclination, or potentially an elliptical galaxy with some residual star formation.
