This galaxy presents as a relatively smooth, centrally concentrated object. Its morphology leans towards an elliptical classification, showing minimal discernible spiral arm structure or distinct disk features. There's an apparent elongation, more akin to an 'in between' rounded and cigar shape rather than perfectly circular. Evidence suggests a minor disturbance in its structure, though not indicative of a major ongoing merger.

The color profile indicates a bias towards older stellar populations, evident from a stronger presence in the redder bands compared to the blue. The central region appears brighter, possibly suggesting a higher density of stars or an active galactic nucleus (AGN), though the resolution prevents confirmation of an AGN. Overall, this galaxy seems to be in a relatively evolved state.
