The galaxy appears as a moderately bright, elongated structure. Its light distribution suggests an elliptical or lenticular morphology, displaying a smooth, centrally concentrated bulge. The galaxy exhibits a significant color gradient, transitioning from a bluer hue in the outer regions to a redder, more luminous core. This color variation may indicate the presence of a central, older stellar population. There are no apparent spiral arms, rings, or other pronounced features typically associated with disk galaxies, suggesting a relatively quiescent star formation history. The overall structure is elongated, but it lacks the distinct distortions indicative of a recent major merger event.
