The galaxy presents as a relatively smooth, elongated structure with a prominent central bulge. Its overall shape is cigar-like, displaying a clear axis of symmetry. There's a distinct color gradient visible, with a reddish hue concentrated within the central bulge, potentially indicating an older stellar population. Fainter blueish regions are observed extending from the central bulge, possibly suggestive of more recent star formation within the galaxy's disk or outer regions. The galaxy appears relatively isolated, showing no obvious signs of major ongoing mergers or tidal disturbances. However, some minor irregularities or slight disturbances cannot be entirely ruled out.
