The galaxy presents as an elongated, cigar-shaped structure. The core exhibits a bright, concentrated luminosity suggesting a significant concentration of stars. There is a color gradient evident from the core outwards; the central region appears more reddish-orange, potentially indicating an older stellar population. Fainter, bluish hues are present in the outer regions, possibly signaling ongoing or recent star formation. The overall morphology is smooth, lacking distinct spiral arms or prominent dust lanes. There are no indications of significant tidal disturbances or ongoing mergers, although subtle asymmetries cannot be ruled out based on this image alone. The galaxy is relatively isolated, exhibiting no nearby companions.