The galaxy appears as a relatively smooth, elliptical-like structure with a concentrated central bulge. There is a radial decrease in luminosity from the center outwards. The color profile suggests a population of older stars, indicated by the yellowish hue, particularly in the central region. There is very little evidence of distinct spiral arms or prominent dust lanes. The galaxy does not appear to be undergoing any major merging events or significant tidal distortions. The overall morphology suggests a galaxy that has largely completed its major star formation phase, but the blue color suggests there are still young stars present. The relatively compact appearance indicates a moderate size for this galaxy.