The galaxy presents as a relatively smooth, centrally concentrated object. There is little evidence of spiral arm structure or prominent dust lanes. The overall shape is somewhat elongated, exhibiting a moderate degree of ellipticity. The color is intermediate, suggesting a mix of stellar populations, with a potential prominence of older stars in the central bulge and younger stars throughout. There is faint asymmetry in the outer regions indicating possible minor gravitational disturbance. The galaxy is a non-interacting field galaxy. Overall the galaxy appears as a non-starburst system with average to lower levels of ongoing star formation.
