The galaxy presents a mixed morphological profile, exhibiting characteristics of both smooth and potentially disturbed features. The primary structure appears largely smooth and centrally concentrated, with a generally rounded shape. There is some irregularity apparent, suggesting a deviation from a perfect elliptical form.

The color profile is not uniform across the galaxy. A central region displays a bluer hue, suggesting a concentration of younger, hotter stars or an active galactic nucleus. This contrasts with a more yellowish or reddish component peripherally, indicative of an older stellar population. 

There is a suggestion of minor tidal disturbances or interactions influencing the morphology, although these features are not particularly prominent. It's plausible this galaxy has undergone a minor merger event in its recent past.