The galaxy presents as a generally smooth object, suggesting a classification leaning towards elliptical morphology. There is minimal evidence of spiral arms or significant disk-like structure. The light distribution appears relatively uniform across the galaxy, lacking distinct features such as star-forming regions or prominent dust lanes. The color profile suggests a population of older stars, contributing to a redder overall hue. The object seems relatively compact, appearing as a concentrated mass of stars. There is a possibility of minor tidal disturbances within the galaxy's structure. Overall the structure has a smooth and rounded appearance, with minimal presence of elongated features. It appears to be a single, unmerged system. Based on the estimated star formation rate, it may be experiencing lower levels of stellar birth activity.
