The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. There is a slight elongation in its overall shape, tending towards an in-between or less rounded appearance. Some evidence of subtle disturbances or irregular features is visible, which may indicate minor gravitational interactions. Overall, the galaxy appears to be of low mass, exhibiting a redder color which suggests a lower rate of star formation and a higher population of older stars.
