The galaxy presents as a moderately bright, elongated system. Its morphology appears to be relatively smooth, but not perfectly so. The light distribution indicates a concentrated central bulge that gradually fades into a diffuse outer disk or halo. The color profile reveals a redder core transitioning to bluer hues in the outer regions, suggesting a difference in stellar populations, with older stars likely dominating the core and younger stars populating the disk. The overall shape resembles an elliptical galaxy, but the slight flattening and color variations could indicate a possible spiral component viewed at a high inclination. There is no apparent evidence of significant ongoing merger activity or major disturbances in the galactic structure.
