The galaxy presents a somewhat smooth morphology with a slightly elliptical shape. The galaxy's core exhibits a bright, concentrated luminosity, possibly indicating a substantial population of older stars or an active galactic nucleus. A subtle, disk-like structure appears to extend outwards from the central region, displaying a bluer hue that suggests regions of ongoing star formation. Overall the galaxy has no major disturbances, but does appear to be undergoing some kind of merging event. The general form of the galaxy exhibits a moderate degree of roundness.