The galaxy presents a generally smooth, elliptical morphology. The central bulge is prominent and appears largely spheroidal with a concentrated luminosity profile. The overall color index suggests an older stellar population, as indicated by the yellow and red hue of the bulge. There is some evidence of a fainter, extended disk component surrounding the bulge, though it lacks well-defined spiral arms. The disk seems to be undergoing some disturbance and possible minor merging as the disk appears distorted. The galaxy's structure suggests it is a relatively massive system with a low star formation rate.
