The galaxy presents a morphology consistent with a spiral galaxy, viewed at a moderate inclination. Two distinct spiral arms are present; they appear somewhat tightly wound around the central bulge region. The central bulge appears moderately prominent. Evidence of a stellar bar is subtle. The outer regions of the disk are less defined, exhibiting a diffuse and fading appearance. The overall color profile suggests ongoing star formation within the spiral arms, contrasting with a more quiescent stellar population in the bulge, and with an overall color profile that suggests it is nearing the green valley, between star forming and quiescent galaxies. The galaxy exhibits a moderate size. No significant tidal disturbances or signs of recent merger activity are discernible. The galaxy lacks a point-like nucleus, indicating the absence of a dominant active galactic nucleus (AGN).
