The galaxy presents an overall elliptical morphology, though its shape deviates somewhat from perfectly round, appearing more elongated. There is a smooth, diffuse light distribution with a bright central bulge. The color gradient suggests a predominantly older stellar population with a concentration of redder stars in the core region. There may be hints of some internal structure, possibly minor tidal disturbances, but these are not very prominent. There appears to be very little dust. Overall, the galaxy seems to be relatively quiescent with some level of ongoing star formation.
