This galaxy exhibits a generally smooth morphology with a slight elongation, appearing somewhat elliptical in shape. It displays a bright central bulge that dominates the overall luminosity, indicating a high concentration of stars in this region. The color profile suggests a relatively older stellar population, with a subtle reddening observed in comparison to galaxies with ongoing, significant star formation. There are hints of a faint, diffuse halo surrounding the central region, although the limited resolution makes it challenging to discern any detailed structures like spiral arms or dust lanes. The overall appearance suggests a galaxy that is not currently undergoing major interactions or mergers, and it is likely in a relatively quiescent state of evolution.
