The galaxy exhibits a generally smooth morphology, suggesting an elliptical or lenticular classification. There appears to be a central bulge, roughly circular in shape, with a notable concentration of light towards the center. The color profile suggests a population of older stars, exhibiting a reddish-yellow hue in the central regions. Moving outwards from the center, the light intensity decreases gradually. There is very little evidence of spiral arms or significant dust lanes; rather, the outer regions appear diffuse and fade into the background. No obvious signs of a major ongoing merger event are visible; however, a subtle asymmetry cannot be entirely ruled out.
