The galaxy appears as a diffuse, low-surface-brightness object. It exhibits a generally elliptical morphology with a noticeable elongation. There is a faint, unstructured haze of light suggesting a relatively smooth distribution of stars. Although the galaxy lacks a clearly defined spiral structure, there are some subtle irregularities hinting at possible disturbances or faint, ill-defined arms. A redder hue toward the core of the galaxy suggests an older stellar population concentrated in the center, with a bluer, fainter halo indicative of younger stars or lower metallicity gas in the outer regions. There is a slight asymmetry to the object, potentially indicative of a minor interaction or past merger event, but the overall smooth texture indicates it is not currently undergoing a major merger.
