The galaxy presents a largely smooth, elliptical morphology. There is a notable absence of prominent spiral arms or a distinct disk structure. The light distribution is concentrated towards the center, indicative of a bulge-dominated system. The galaxy appears remarkably rounded, showing no significant elongation or asymmetry. There is no evidence of any ongoing major merging events or strong tidal disturbances. A faint yellowish hue is visible which may indicate an older stellar population with limited ongoing star formation.
