The galaxy presents a generally smooth morphology, with a somewhat elliptical shape. Its light profile appears concentrated, lacking prominent spiral arm structures or strong irregularities. The observed color suggests a relatively older stellar population, with less recent star formation compared to bluer, star-forming galaxies. There is a slight elongation to the object, and a subtle color gradient may exist with a slightly bluer core. No distinct dust lanes or other features disrupting the smoothness of the overall light distribution are readily apparent within the available image resolution.
