The galaxy presents as a relatively smooth, centralized object with a slight elongation. It appears to be a disk galaxy at a relatively small inclination. The light profile suggests a dominant bulge component and/or possible bar structure, with a more diffuse, less prominent disk. There is a higher likelihood of a smooth morphology, yet some features or subtle structure are still possible. The inner regions exhibit a yellowish hue, possibly indicating an older stellar population or dust obscuration. The outer regions appear slightly bluer, suggesting the presence of some younger stars and potential star formation, although the overall rate of star formation appears moderate. There is no obvious evidence of a major merger in progress, though the possibility of minor disturbances or past merger events cannot be ruled out. It is approximately 7 kpc in size. The galaxy is luminous.