The galaxy presents as a somewhat elliptical, largely featureless object with a smooth light distribution. There is a central concentration of light, indicative of a possible galactic bulge. The galaxy displays a color gradient; its core appears to be a pale yellow-white, with a subtle shift towards a bluer hue towards the outer edges. This color profile might suggest a population of older stars in the central bulge, with younger, bluer stars populating the disk. The galaxy does not show any strong evidence of spiral arm structure or active star formation regions, and does not appear to be strongly disturbed or interacting with other galaxies. The galaxy's structure appears to be relatively well-ordered and settled.