The galaxy presents as a slightly elongated, lenticular structure. Its overall color profile exhibits a yellowish-white hue, suggesting a relatively older stellar population with lower ongoing star formation. The galaxy's light is concentrated towards the center, implying a significant bulge component. The disk appears relatively smooth and lacks prominent spiral arm features. There is only some very faint blue in the galaxy, likely caused by faint ongoing star formation. The galaxy does not show any evidence of major tidal disturbances or ongoing mergers, though there is some slight asymmetry to the disk. Overall, this galaxy appears as a settled, relatively massive system.
