The galaxy presents as a smooth, elliptical structure. It appears elongated, approximately cigar-shaped, with a bright, concentrated core. The light distribution suggests a relatively featureless morphology, lacking prominent spiral arms or distinct dust lanes. Color gradients are subtle, with the central region exhibiting a slightly yellowish hue, potentially indicative of an older stellar population. The outer regions appear somewhat bluer, suggesting the presence of some younger stars, though this is not as obvious as the yellow hues. There is no strong evidence of any ongoing major mergers or significant tidal disturbances in the immediate vicinity.
