The galaxy presents as a lenticular or possibly elliptical galaxy due to its smooth, generally featureless appearance. The galaxy exhibits an elongated morphology, approximating a cigar shape. It is predominantly a yellow-orange hue, which suggests a stellar population dominated by older, redder stars, indicating a relatively low rate of current star formation. There is no evidence of prominent spiral arms or dust lanes. There is a slight indication of a faint extended halo surrounding the brighter central region, but it lacks distinct features. There is no visual evidence of active galactic nuclei activity. The galaxy appears relatively undisturbed, with no signs of ongoing major mergers or tidal disruptions.
