The galaxy presents a generally smooth, elliptical morphology with a high degree of central concentration. The light profile appears to be dominated by an older stellar population, indicated by the yellow-red hue. There is no evidence of spiral arms, distinct disk features, or ongoing major mergers. A slight elongation is visible, suggesting it is not perfectly spherical. Faint, diffuse outer regions are present, but the galaxy lacks significant tidal disturbances or asymmetries. The overall structure suggests a relaxed system, likely an evolved galaxy that has undergone significant internal processing. Star formation appears low.
