The galaxy presents as a single, fairly smooth and rounded object with a dominant central bulge. The color profile indicates an older stellar population, with a yellowish-orange hue dominating the central region. There is some faint bluer light visible, possibly indicating some regions of more recent star formation, particularly in the outer regions of the galaxy. There appears to be a very slight asymmetry, but no obvious spiral arm structure or signs of significant tidal disturbance or major merging events. The galaxy is slightly elongated, appearing more like a disk or a rounded elliptical. Overall, the galaxy appears to be a relatively undisturbed, massive system, with a primarily old stellar population and hints of ongoing, low-level star formation.
