The galaxy presents as a luminous, elliptical object with a slightly elongated morphology. A bright central bulge is prominent, exhibiting a yellowish hue indicative of an older stellar population. The bulge gradually fades into a surrounding, more diffuse disk. Hints of bluer regions are observed in the outer disk, suggesting the presence of younger, hotter stars and regions of active star formation, though these are not strongly pronounced. The overall structure appears relatively smooth, lacking significant spiral arm structures or prominent dust lanes. The galaxy exhibits a notable tilt relative to our line of sight, providing a view of its discal structure.
