The galaxy presents an elongated, cigar-shaped morphology. Its central region exhibits a smooth, concentrated appearance with a yellowish-orange hue, suggestive of an older stellar population. Moving outward from the center, a faint, diffuse disk is discernible, tinged with blue hues along the edges, potentially indicative of ongoing star formation within a relatively low star formation rate. There is no apparent presence of spiral arms or significant dust lanes visible within the galaxy's structure. No signs of major mergers or substantial tidal disturbances are apparent; however, there are hints of minor disturbances that are possibly mergers.
