The galaxy presents as a somewhat elliptical, smoothly distributed light source. The core region appears bright and concentrated, with a yellowish hue, suggesting a population of older stars. Surrounding the central bulge, a more diffuse, slightly bluer region is visible, indicating the presence of some younger stellar populations and potential ongoing star formation. No distinct spiral arms or bar structures are discernible. A subtle asymmetry is hinted at in the outer regions. Overall, the galaxy appears to be an early-type system undergoing a moderate level of star formation.
