The galaxy presents an elliptical morphology, appearing elongated and cigar-shaped. It exhibits a smooth, featureless structure with no apparent spiral arms or prominent dust lanes. The central region displays a higher concentration of light, suggesting a dense nucleus. The galaxy's color gradient shifts from a bluer hue at the edges to a redder tint towards the core, potentially indicating a population of older stars dominating the central region, with younger stars distributed more diffusely within the galaxy's halo. There is a possible minor companion galaxy nearby, but it does not appear to be undergoing a major merger. There are no major disturbances to the galaxy's shape.
