The galaxy appears to be a relatively smooth, elliptical-like structure with a concentrated central bulge. There is a generally spheroidal morphology, although it is not perfectly circular. Its light distribution suggests a lack of significant spiral arms or distinct features typically associated with late-type spiral galaxies. The galaxy exhibits a predominantly yellow-orange hue, suggestive of an older stellar population and/or dust obscuration. There may be some low-level disturbances, but the overall structure is generally quiescent. The galaxy appears relatively isolated, with no other bright galaxies in close proximity suggesting a recent merger.
