The galaxy presents an overall ellipsoidal morphology, suggesting an evolved system. The light distribution is concentrated towards the center, with a relatively smooth appearance indicative of an older stellar population. There is a hint of asymmetry in the isophotes, possibly indicative of a past minor merger event. The galaxy exhibits a distinct color gradient, with the central regions appearing redder, which may point to a population of older, redder stars. The outer regions exhibit a bluer tint, potentially due to the presence of a younger stellar population or ongoing star formation. The system is estimated to have an effective radius of approximately 3 kpc. The overall shape is somewhere in between round and cigar shaped, but closer to round. Evidence suggests that the system is undergoing some sort of disturbance from another object nearby.
