The galaxy presents a moderately concentrated light profile, appearing somewhat elliptical in shape. There is a suggestion of a central bulge or core region that exhibits a yellowish-orange hue, indicating a population of older stars. Surrounding this core, a less defined and bluer area suggests some disk-like structure or extended stellar population. This region exhibits evidence of ongoing or recent star formation, contributing to its bluer color. No distinct spiral arms or prominent dust lanes are visible in this image. The overall texture of the galaxy's light distribution appears relatively smooth, although there are hints of possible minor disturbances or irregularities in its morphology. The galaxy does not show any strong indications of a major ongoing merger but a possibility of a minor disturbance exists.
