The galaxy presents as a moderately bright, elongated structure. Its light profile appears relatively smooth, lacking the distinct spiral arms or bar-like features characteristic of grand design spiral galaxies. The central region, or bulge, is discernible as a concentrated area of brighter light, fading outwards into the outer regions of the galaxy. The galaxy exhibits a slight tilt relative to our line of sight, as indicated by its non-circular appearance. There are hints of substructure or minor irregularities in the outer regions, potentially indicative of past interactions or ongoing accretion events, although the resolution limits detailed analysis of these features. The overall color appears yellowish-white, suggesting a stellar population dominated by older, cooler stars. The galaxy is reasonably compact.
