The galaxy appears to be relatively small in angular size. The light profile suggests a compact morphology. The overall color of the galaxy is notably red, indicating a significant population of older stars and/or a high level of dust obscuration, which are impacting the transmission of blue light. The galaxy's morphology is not obviously disk-like or spiral in nature. There is a slight asymmetry that may indicate a minor disturbance. No clear evidence of a recent major merger is apparent, though the asymmetrical shape suggests potential gravitational interaction with a nearby object. There appears to be a faint surrounding halo or envelope.
