The galaxy presents as a relatively small, elliptical-like structure with a smooth, diffuse appearance. The light distribution suggests a concentration of stars towards the central region, fading outwards into a less dense halo. There is little evidence of spiral arms or prominent dust lanes. The overall color profile is a consistent bluish hue, indicating a possible population of younger, hotter stars, although this may be a slight artifact. There is no major interaction or obvious merging event occurring. The galaxy appears largely undisturbed. There's potentially some slight warping of the disk.