The galaxy presents as a relatively smooth, elliptical-like structure. There is a concentration of light towards the center, suggesting a prominent galactic bulge. The outer regions appear to gradually fade, with no distinct edges or spiral arm structures visible. The color profile indicates a redder central bulge transitioning to slightly bluer hues in the outer regions. This color gradient potentially reflects variations in stellar populations, with older, redder stars dominating the bulge and younger, bluer starsPopulating the outer disk. No significant dust lanes or signs of ongoing major merger activity are apparent; it appears mostly undisturbed. A slight elongation is visible, suggesting that the galaxy is not perfectly spherical, it may be cigar shaped, but close to in between round and cigar shaped. The galaxy is not perfectly smooth, but close.
