The galaxy presents as a well-defined, elongated structure. Its light profile appears relatively smooth, suggesting a dominant spheroidal component. The central region exhibits a concentration of light, possibly indicating a bulge or active galactic nucleus. The color of the galaxy appears reddish-yellow, hinting at an older stellar population. The overall morphology is consistent with an elliptical galaxy, with no discernible spiral arms or significant star formation regions. There is some indication of a minor disturbance in the symmetry of the galaxy, perhaps suggesting a past or ongoing interaction.
