The galaxy presents as a generally smooth, elliptical-like structure with a concentrated central bulge that emits a yellow-orange hue. The light profile suggests a high degree of spherical symmetry. There is a subtle color gradient, with the central region appearing slightly warmer in color than the outer regions. Faint traces of what could be a very weak disk are visible near the central region of the galaxy, as there are some patches of light that look like they could be arms. No major disturbances or tidal features are immediately apparent, indicating that it is not currently undergoing a major merging event. The lack of strong blue emission suggests a relatively low ongoing star formation rate. Overall, the galaxy appears to be a quiescent, massive system with a relatively old stellar population, with a redshift of 0.374077.
