The galaxy presents as a moderately luminous, disk-shaped system with an apparent elongated morphology. Its central region exhibits a yellowish-white hue, suggesting an older stellar population dominating the core. Moving outward from the center, a subtle blue tinge is observed, potentially indicative of more recent star formation in the outer regions of the galactic disk. There is little evidence of strong spiral arm structure within the disk; instead, the structure appears relatively smooth. Subtle irregularities are present, which may be suggestive of minor gravitational interactions or internal dynamic processes. The object appears to be well-resolved. Based on color, the object appears to be relatively passive.
