This galaxy appears to be an elliptical or lenticular type, presenting a generally smooth and centrally concentrated light distribution. The core region exhibits a bright, yellowish hue, which likely corresponds to an older stellar population. A faint and diffused disk-like structure surrounds the core, with a subtly elongated shape, suggesting a possible disk component viewed at an angle. No distinct spiral arms or active star-forming regions are apparent in the imagery. There may be minor evidence of past interactions or disturbances as the light is slightly asymmetric around the halo. The color profile suggests a relatively quiescent galaxy with ongoing low levels of star formation, and is of intermediate to high mass.
