The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge, characterized by a yellow-orange hue, suggesting an older stellar population. There is little evidence of significant star formation within the bulge. The galaxy appears relatively undisturbed, lacking any signs of major mergers or tidal distortions. A faint, diffuse halo surrounds the central region, gradually fading into the background. The lack of distinct spiral arms or features indicates a classification leaning towards an elliptical type.
