The galaxy appears as a relatively smooth object. It exhibits a slightly elliptical morphology, with a notable concentration of light towards its center, suggesting a prominent bulge. There is a distinct absence of well-defined spiral arms or a clear disk structure, however, there is a subtle hint of possible disk-like features. The color appears largely uniform across the galaxy, trending towards the redder end of the spectrum. This redder hue implies a stellar population dominated by older, redder stars, consistent with a relatively low ongoing star formation rate. While a generally smooth appearance prevails, there may be some subtle signs of minor disturbances in the galaxy's morphology, hinting at potential past interactions. The general morphology would suggest that this galaxy can be classified somewhere between an elliptical and lenticular galaxy.
