The galaxy presents a generally smooth morphology, appearing largely spheroidal in shape, with a suggestion of intermediate ellipticity rather than perfectly circular or elongated. There is a dominant central bulge, which appears bright and somewhat diffused. Faint, extended features or a disk component may be present but are difficult to resolve clearly given the resolution of the image. There may be some evidence of minor disturbances or tidal features, but the overall structure seems relatively undisturbed, and a current major merger event is not apparent. The light distribution is concentrated towards the center, consistent with a more evolved stellar population. There are no prominent, bright star-forming regions immediately visible. The overall color is somewhat redder, suggesting a lack of significant ongoing star formation, consistent with a higher fraction of older stars.
