The galaxy appears as a fairly smooth, concentrated object. Its overall shape is somewhat elliptical but not perfectly round, leaning towards an intermediate spheroidal form. There is a slight asymmetry suggesting a possible minor gravitational disturbance or interaction. The color profile reveals a central yellowish hue surrounded by a bluer outer region. This color distribution indicates some ongoing star formation activity, especially in the outer parts. There is no evidence of a significant central bulge or prominent spiral arms. The light distribution appears relatively concentrated, suggesting a substantial mass density in the central region.
