The galaxy presents as a somewhat elliptical structure, with a discernible bulge that appears significantly brighter and more concentrated than the surrounding disk. The galaxy exhibits a relatively smooth texture, with a gradual decline in surface brightness from the core outwards. There is subtle color variation. The central bulge displays a yellowish hue, potentially indicating an older stellar population, while the outer regions show hints of bluer tones, suggestive of some ongoing, albeit subdued, star formation activity. The overall morphology suggests the galaxy is not undergoing any major mergers, although minor disturbances can't be completely ruled out. The elongated shape is suggestive of a disk component viewed at an oblique angle. The estimated size is about 4.8 kpc across.