The galaxy presents as a lenticular or elliptical galaxy, exhibiting a smooth, concentrated morphology with a high degree of central concentration. It has an elongated shape and is highly inclined from our viewpoint, presenting as cigar-shaped. There are no distinct spiral arms or prominent features indicative of ongoing major mergers or significant tidal disturbances. There might be a very minor perturbation within the galaxy structure itself, but that cannot be determined with certainty. The object shows a redder hue, possibly indicating an older stellar population with low levels of current star formation. The object is moderately bright, suggesting a medium sized galaxy.
