The galaxy presents as a somewhat elliptical structure, with a bright, concentrated central bulge. The outer regions of the galaxy appear more diffuse, fading gradually into the background. The color profile indicates a relatively even distribution of stellar populations across the visible spectrum, with a slight tendency toward bluer tones in the outer regions compared to the yellower central bulge. The shape is more in-between rather than completely round, or cigar shaped. There is a slight hint of asymmetry suggesting a possible gravitational interaction or minor disturbance, but overall the morphology suggests an isolated system. No evidence of a major merger is seen in the immediate vicinity. The surface brightness distribution appears relatively smooth, indicative of a fairly evolved system with less active star formation than galaxies with prominent spiral arms or irregular features.
