The galaxy presents as a relatively smooth, centrally concentrated light distribution. It exhibits a roughly elliptical morphology, appearing somewhat elongated rather than perfectly circular. There is a noticeable color gradient, with the central region exhibiting a brighter, more whitish-blue hue, suggestive of a population of hotter, younger stars. Moving outwards from the core, the galaxy becomes fainter and appears slightly redder, potentially indicating an older stellar population. No distinct spiral arms or other features are readily discernible, giving it a generally smooth appearance. There's no clear evidence of a major ongoing merger or significant tidal disturbance, although there may be a subtle asymmetry in the outer isophotes. The overall impression is that of an early-type galaxy, possibly an elliptical or lenticular, at a moderate redshift.
