The galaxy presents as a slightly elongated, disk-like structure. The central region exhibits a bright, concentrated core, suggesting the presence of a galactic nucleus. The luminosity appears to gradually diminish from the core outwards.

The galaxy displays a subtle color gradient, with a hint of bluer tones in the outer regions, potentially indicative of ongoing star formation. The inner region appears comparatively redder, possibly due to an older stellar population and/or dust obscuration.

There is a slight suggestion of possible minor disturbances in the galaxy's form, with a subtle asymmetry to the structure. This warrants closer inspection to determine if there is interaction or merging with another galaxy.
