The galaxy presents with a generally elliptical morphology, though it shows some irregularities suggesting potential interactions or internal disturbances. The central region exhibits a bright, concentrated core, which appears yellowish-white in color. Surrounding the core is a more diffuse halo or bulge component, showing a wider range of colors, including blue and red gradients. This suggests a complex stellar population within the galaxy, possibly indicating ongoing star formation or varied stellar ages and metallicities. There appears to be some degree of distortion within the outer regions of the galaxy, which could indicate a minor merger event. Overall, the galaxy displays a moderately disturbed morphology and complex stellar population.
