The galaxy presents as a moderately luminous object, displaying a distinct elongated, cigar-like morphology. The light distribution appears relatively smooth and concentrated, with a noticeable lack of distinct spiral arms or prominent dust lanes. There is a suggestion of a disk structure, but it appears subdued. The galaxy's color is generally consistent across its visible extent, though the central region may appear slightly redder than the outer regions. There is no obvious indication of ongoing major merger activity, although minor disturbances cannot be ruled out. Overall, the galaxy appears to be a relatively evolved system, likely with a significant stellar mass and a moderate rate of star formation.
