The galaxy presents as a relatively luminous, elongated structure. The central region exhibits a high degree of concentration with a yellowish hue, suggesting an older stellar population is dominant in the core. Extending outward from the core, there appears to be a flattened disk-like structure. The disk does not appear to exhibit strong spiral arm features. The edges of the galaxy fade gradually into the background sky, indicating a smooth transition in stellar density. There may be a slight warp or disturbance in the galactic plane on one side, suggestive of a possible interaction or past merger event, however, this could also be an artifact of the viewing angle. The lack of prominent blue regions indicates a lower rate of recent star formation. Overall, the galaxy appears to be a relatively massive system with a moderately evolved stellar population.
