The galaxy presents a distinctly elongated, cigar-shaped morphology. The light distribution appears relatively smooth, suggesting a possible elliptical or lenticular classification. A subtle color gradient is observable, with the central region exhibiting a warmer, reddish hue, which may indicate an older stellar population and/or the presence of dust. The outer regions show hints of a bluer component. I cannot discern distinct spiral arms or a well-defined disk structure. No obvious signs of major merger activity are present, although subtle asymmetry or minor distortions could be indicative of tidal interactions or past merger events. Overall, the galaxy gives the impression of a fairly quiescent system with a moderate mass and star formation rate.
