The galaxy presents a generally smooth and rounded morphology. A bright, concentrated central bulge dominates the structure, displaying a yellowish-orange hue, suggesting an older stellar population with minimal ongoing star formation. The surrounding envelope appears less defined with a slightly redder tint that gradually diffuses outwards, with little evidence of spiral arm structures or prominent dust lanes. The galaxy appears relatively undisturbed, exhibiting minimal signs of tidal interactions or mergers. Overall, the galaxy appears to be an elliptical galaxy with a fairly concentrated stellar distribution.
