The galaxy presents as a largely featureless, smooth structure, with a concentrated central region exhibiting a yellowish hue. This central concentration appears spheroidal, suggesting a significant bulge component. The galaxy displays a high degree of roundness in its overall shape. There is a very slight indication of a possible minor disturbance or interaction event in the outer regions of the galaxy, though not clearly evident. The faintness of the outer regions compared to the central concentration may indicate an older stellar population in the galaxy's periphery. There is no readily apparent spiral arm structure visible.
