This galaxy exhibits a generally smooth morphology with a discernible, elongated shape. The galaxy's light distribution appears concentrated towards the center, suggestive of a prominent bulge. There is evidence of a disk component, although it is not sharply defined. The primary color is a yellowish-white hue, possibly indicative of an older stellar population, with traces of bluer regions, potentially hinting at younger star formation. There are no clear signs of major disturbances or mergers. The overall structure suggests a galaxy somewhere on the elliptical-spiral spectrum, leaning towards a lenticular type.
