The galaxy presents as an elongated, cigar-shaped system with a smooth morphology. The central region exhibits a bright, concentrated luminosity profile, suggesting a significant stellar population density. Moving outward from the center, the light appears to diminish gradually, indicating a smooth transition to the outer regions. There is a slight color gradient visible, with the central region appearing more yellow/orange, possibly indicating an older stellar population. The outer edges of the galaxy seem to have a slightly bluer hue, which could indicate the presence of younger, hotter stars or a lower metallicity. No distinct spiral arm structures or prominent dust lanes are discernible from this image. There is no obvious evidence of a major merger or strong tidal disturbance affecting the galaxy's overall structure, however, there is possibly some minor irregularity in the distribution of light that could be indicative of a recent or ongoing minor interaction.
