The galaxy appears to be a relatively large, luminous system, exhibiting a central bulge that dominates its overall structure. The bulge displays a smooth, concentrated morphology, with a yellowish hue indicating a potentially older stellar population.  Extending from the bulge is a faint, diffuse disk.  The disk presents a bluer color, suggesting the presence of younger, hotter stars. The overall shape appears more elliptical, being only subtly elongated. There are no strong indications of active star formation in the nuclear region, though faint hints of star formation may be present in the disk. There is no evidence of major mergers or strong tidal features, although minor asymmetries or disturbances cannot be ruled out in the disk. The galaxy appears relatively isolated, with no clear signs of strong interactions with neighboring galaxies.
