The galaxy exhibits a predominantly smooth morphology with a concentrated central bulge. The bulge displays a yellow-orange hue, potentially indicative of an older stellar population. The surrounding galactic disk is less distinct but has a subtle presence. This region exhibits a color gradient moving from a faint red to a deeper blue farther from the center. The galaxy’s shape appears to be primarily elliptical or lenticular, with a relatively high degree of roundness. There is no strong evidence of spiral arm structure or significant tidal disturbances. The galaxy seems relatively isolated with no obvious signs of ongoing or recent major mergers. There is a hint of slight asymmetry in the outer region.