The galaxy presents as a slightly tilted disk-shaped system, approximately 4.5 arcseconds in diameter. The central region exhibits a bright, concentrated bulge. The bulge has an ellipticity of 0.39, with the major axis position angle around 80 degrees. The galaxy appears to be a spiral type, with hints of spiral arm structure, although these are not sharply defined. There is evidence of possible minor tidal disturbances or interactions, suggested by the slightly irregular shape of the disk. The overall color profile suggests a modest amount of recent star formation, particularly in the outer regions of the disk, but the bulge exhibits a redder hue, indicating an older stellar population. The galaxy displays an inclination that is approximately 60 degrees from face on.
