The galaxy presents as a relatively smooth, elongated structure, suggestive of a disk galaxy viewed at a high inclination. Its overall color appears to be bluish-white, possibly indicating a population of young, hot stars. There's a subtle color gradient, with the central region exhibiting a slightly redder hue compared to the outer edges, which may be due to a higher concentration of older stars or dust extinction toward the core. There is no evidence of any major mergers, but there appears to be a slight irregularity that may represent some minor disturbance.
