The galaxy presents an elongated, elliptical morphology. The core region exhibits a bright, concentrated luminosity, suggestive of a significant stellar density and potentially a centrally located active galactic nucleus. There is an asymmetric distribution of light with a slightly brighter lower section. The overall color profile indicates a presence of both older stellar populations, noted through redder hues, and regions of active star formation characterized by bluer tints. There is a noticeable disturbance or merging event appearing to be underway, as evidenced by the irregular light distribution and extended structures emanating from the central region. The faint and diffuse outer regions suggest a relatively large effective radius.
