The galaxy appears as a moderately bright, elliptical system with a concentrated central bulge. The overall shape is elongated, displaying an intermediate ellipticity. The light distribution suggests a relatively smooth profile, transitioning from a bright core to a fainter, diffuse outer region. There's a subtle color gradient visible, with the central regions appearing slightly yellower compared to the bluer hues in the outskirts. This indicates potential variations in stellar populations across the galaxy, possibly with older stars concentrated toward the center and younger stars in the outer regions. The orientation of the galaxy is approximately tilted with respect to the line of sight. There's no prominent evidence of spiral arms or significant dust lanes. Overall, the galaxy presents as a relatively undisturbed, mature system.
