The galaxy presents as a relatively smooth, centrally concentrated object with a subtle disk-like morphology. The core is a bright, yellowish hue, indicative of an older stellar population. The outer regions exhibit a slightly more diffuse and less structured appearance. There is a hint of a possible minor interaction or disturbance visible in the periphery, with a very faint and small object very close to the galaxy with a red hue, suggesting a lower level of star formation relative to the main galaxy body. The primary galaxy has a largely smooth structure, with the majority of the population having a smooth distribution. The overall shape appears to be in between round and elongated, but is closer to round. There are only subtle signs of any mergers, with a slight distortion in the edge.
