The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a largely elliptical morphology, appearing quite round with only a slight deviation towards a cigar shape. There's a noticeable color gradient, with a yellowish hue dominating the core region, suggestive of an older stellar population concentrated towards the center. Moving outward from the core, the light transitions to a slightly bluer color which may indicate the presence of younger stars within the outer regions.

There's little evidence of prominent spiral arms or distinct disk features. No significant tidal tails or obvious signs of a major merger event are observed, though there may be slight minor disturbances in the outer halo. The smooth appearance suggests that star formation rate might be low.
