The galaxy presents a predominantly smooth, elliptical morphology. It is a relatively bright object with a concentrated central bulge exhibiting a yellowish hue, indicative of an older stellar population. The galaxy appears to be slightly elongated with a generally round shape, but tends more toward being in between round and elongated. There is a subtle, faint disk-like structure surrounding the core region. There are no distinct spiral arms or prominent dust lanes visible within the disk. The overall structure suggests a fairly quiescent galaxy, with no major disturbances visible. There are suggestions of disturbances on the lower left of the galaxy. No apparent merger is occuring.
