The galaxy presents as an elongated, cigar-shaped structure with a relatively smooth appearance. The light distribution suggests a central bulge that transitions into a disk, though no spiral arm structures are clearly discernible. The galaxy displays a color gradient, appearing more yellow/orange toward the center, indicative of an older stellar population, and transitioning towards a bluer hue at the edges which may be an area with more active star formation. There are no obvious signs of a major ongoing merger or significant tidal disturbances, though minor irregularities in the shape cannot be ruled out at this resolution. The galaxy appears to be relatively isolated within its immediate environment.
