The galaxy presents as a somewhat diffuse object with a moderately concentrated central region. There is an absence of clearly defined spiral arms or a prominent bar structure. The overall shape appears roughly elliptical, although some irregularities suggest potential disturbances. The colour profile indicates a higher concentration of older stellar populations, particularly towards the central bulge, which exhibits a redder hue. The outer regions show slightly bluer tones, potentially indicating more recent star formation, but star formation is occurring at a low rate overall. While the galaxy appears generally smooth, subtle asymmetries and distortions hint at possible past or ongoing interactions, but the galaxy is generally not undergoing significant merging activity. 
