The galaxy presents as a largely featureless elliptical or lenticular-like object, exhibiting a smooth, centrally concentrated light distribution. The core displays a bright, yellowish-orange hue, indicating a population of older stars and a dearth of active star formation in that region. The isophotes appear to be approximately circular, suggesting a generally relaxed morphology. There is little evidence of spiral arms, dust lanes, or other distinct structural features. A faint, diffuse halo of light extends outwards from the central region. No signs of an active galactic nucleus are apparent from this observation. Based on morphology, this galaxy is likely on the red sequence.
