This galaxy presents a predominantly smooth morphology. It exhibits a central concentration of light, suggesting a substantial bulge component. The overall shape appears somewhat elongated, but not strongly so; tending towards a more rounded appearance. There is some evidence of possible minor disturbances or interactions, indicated by subtle asymmetries or irregularities in the outer regions, although a clear merger is not obvious. The color profile is fairly uniform across the galaxy, with a slight redder tint overall, suggestive of an older stellar population and/or dust obscuration, though there are subtle signs of recent star formation.
