The galaxy appears to be a relatively smooth, disk-like system, viewed at an oblique angle. Its light profile suggests a centrally concentrated bulge, with a surrounding, less luminous disk component. The galaxy exhibits a subtle colour gradient, transitioning from a slightly bluer hue in the outer regions of the disk to a more neutral colour towards the central bulge. There is no strong evidence of spiral arm structure or significant star formation activity within the disk. The overall morphology suggests a relatively evolved system, potentially with ongoing but subdued star formation. There is a slight indication of minor structural asymmetry, which may be indicative of a past or ongoing interaction. No obvious merging companion galaxy is apparent in the immediate vicinity.
