The galaxy presents as an elongated, cigar-shaped structure with a discernible disk. The overall color profile suggests relatively evolved stellar populations, with a redder hue dominating. There is evidence of a smooth distribution of light across the galactic body, indicating a lack of prominent spiral arms or intense star-forming regions. However, some subtle variations in color and brightness within the disk might imply localized star formation, albeit at a low rate. The galaxy shows no obvious signs of major mergers, with no large tidal tails or strongly distorted morphology observed. Any interactions appear to be minor, given the integrated smooth light profile.
