The galaxy presents a generally smooth morphology with a centrally concentrated luminosity profile. The light distribution is relatively uniform, lacking distinct spiral arm structures or prominent features suggestive of recent major mergers or tidal interactions. The overall shape appears close to circular, with only slight deviations from perfect rotational symmetry. There is a noticeable color gradient, exhibiting a more reddish hue toward the central regions, which transitions to bluer colors in the outer regions. This color gradient suggests a possible difference in stellar population, where older, redder stars dominate the core, with younger, bluer stars in the outskirts. The inferred low star formation rate may point toward a more passive evolution.
