The galaxy presents as a relatively smooth, centrally concentrated structure with a generally elliptical morphology. The color gradient transitions from a more blue-ish hue at its core to a redder, yellower color in the outer regions. There is no clear evidence of spiral arms or a well-defined disk structure; the overall appearance suggests a more spheroidal or lenticular system. Faint irregularities are present along the edges, possibly indicating minor disturbances. The dominant component appears to be a relatively old stellar population.
