The galaxy presents as a primarily smooth object, though some features are discernable upon closer inspection. The central region exhibits a bright, concentrated core that transitions into a more diffuse surrounding halo. The shape appears largely rounded, with only a minor deviation towards an elliptical form. 

There is evidence suggesting the presence of a minor disturbance or asymmetry within the galaxy's structure. While the overall morphology is not indicative of a major merger, a subtle irregularity in the distribution of light hints at possible past interactions or internal dynamic processes.

The color profile reveals a general trend where the central region is significantly more yellow, while outer regions appear cyan or blue. This likely corresponds to a difference in stellar populations. This is consistent with older stellar populations concentrated in the core and younger populations in more disc-like or outlying regions.
