The galaxy presents as an elongated, elliptical morphology, potentially exhibiting a cigar-like shape. There is a smooth light distribution throughout the galaxy body, with an apparent lack of distinct spiral arm structures or prominent dust lanes. The color gradient shifts from a more yellowish hue at the center to a bluer tone at the outer edges. This suggests a likely concentration of older stellar populations toward the core and younger star formation activity in the periphery. There is no evident morphological evidence suggesting recent major mergers or significant tidal disturbances. Light seems to be more concentrated towards the central area.
