The galaxy presents as a centrally concentrated object with a generally smooth appearance, exhibiting an elliptical morphology. The light distribution suggests a structure that transitions gradually from a bright nucleus to a fainter outer region. There is no evidence of strong spiral arms or a distinct disk structure. Color gradients across the galaxy suggest a change in stellar population with radius, possibly with older, redder stars dominating the outer regions and bluer stars in the center. The galaxy appears relatively undisturbed, without any significant signs of ongoing major mergers or tidal interactions with other galaxies.
