The galaxy presents an elongated, somewhat disturbed morphology, suggestive of a system undergoing interaction or exhibiting internal instabilities. It appears to be largely spheroid in shape. Its color profile indicates a mix of stellar populations, with a dominant yellowish-orange hue indicative of older stars, but there appears to be some bluer elements indicating some star formation is occurring. There also appears to be a tidal tail or stream extending from the central body. The system exhibits low-level disturbances within its structure, hinting at a past or ongoing interaction. The galaxy displays a considerable degree of asymmetry, adding further evidence of its dynamic state. There is some clumpy structure visible across the galaxy, though it is hard to define clearly.
