The galaxy presents as an elongated, cigar-shaped structure. It exhibits a smooth, centrally concentrated luminosity profile, with the light appearing to fade gradually towards the edges. There is a subtle color gradient visible, with the central regions appearing more yellow-orange, which could indicate an older stellar population or the presence of dust. The outer regions exhibit a slightly bluer hue, suggesting the presence of some younger, hotter stars. The absence of strong, well-defined spiral arms or a prominent disk indicates a relatively featureless morphology. There are no obvious signs of recent major merger events, although some minor disturbances cannot be entirely ruled out at this resolution. Overall, the galaxy appears to be a relatively evolved system.
