The galaxy presents as a centrally concentrated object, exhibiting a smooth overall morphology. Its color profile indicates a dominant yellowish hue in the central region, suggesting a likely older stellar population. This central concentration appears elliptical in shape, transitioning gradually to a fainter, somewhat bluer, extended halo. There is a slight asymmetry in the outer region, possibly hinting at minor tidal disturbances or interactions, though no strong evidence of major merging events is immediately apparent.
