The galaxy presents as a single, relatively homogenous structure. Its overall color appears to be a fairly uniform blue-white hue, suggesting a moderate to high population of younger stars. There is little visible differentiation in color or texture across the body of the galaxy, implying a lack of defined spiral arms or a prominent bulge component. Its shape is generally elliptical, nearing circular, with no obvious distortions or tidal features indicative of recent major mergers. The light distribution is relatively smooth, lacking any bright knots of star formation or evidence of significant dust lanes. Based on the absence of prominent features, the galaxy is likely an elliptical galaxy.
