The galaxy appears as a single, largely featureless object, exhibiting a smooth, elliptical morphology. It is centrally concentrated with a gradual decrease in luminosity outward from the core, the galaxy appears to be mostly spheroidal in shape. The color profile suggests an older stellar population, with the dominant light likely emitted by redder, evolved stars. There is no clear evidence of spiral arms, dust lanes, or active star formation regions within the observed bands. Minor asymmetry or irregularity is not apparent within the limits of resolution. The galaxy is isolated.
