The galaxy presents a distinctly elongated, cigar-like morphology. Its light profile suggests a relatively smooth overall structure, with a centrally concentrated brightness gradient. A subtle color gradient is observable, transitioning from a redder hue in the central bulge to a somewhat bluer tint in the outer regions. There appear to be weak disk-like structures, but this is not certain. There is no obvious evidence of tidal features or ongoing major mergers. Subtle asymmetry may exist, but this is difficult to assess given the image resolution.
