This galaxy appears to be an elliptical or lenticular type, exhibiting a generally smooth and centrally concentrated morphology. The light distribution suggests a dominant bulge component with a gradual falloff in brightness with increasing radius. The galaxy has a slight elongation, not perfectly spherical, and displays a yellowish-white hue, suggestive of an older stellar population. There is no discernible evidence of prominent spiral arms or ongoing major mergers; however, the outer regions exhibit subtle irregularities that could indicate minor disturbances or past interactions. Star formation activity appears subdued, aligning with the color and smooth, featureless appearance. Overall, it presents a relatively evolved and settled system.
