The galaxy presents as an elliptical or lenticular type, exhibiting a generally smooth morphology. There is a bright central bulge or core with a relatively smooth light distribution, suggesting an older stellar population and minimal ongoing star formation in the galaxy's center. The outer regions display a slightly more irregular structure and a bluish hue. The galaxy shows little evidence of spiral arms or disk features, instead exhibiting a more spheroidal appearance. Faint extensions or tidal features are noted around the galaxy, potentially indicating past or ongoing interactions or minor disturbances. There is a subtle color gradient, with the central regions appearing slightly redder than the outer parts, which exhibit a bluer tint. This color variation may indicate differences in stellar population ages or dust content.