The galaxy presents as a relatively smooth, elliptical-like structure, though it is not perfectly spherical. There is a suggestion of a slight elongation, giving it a somewhat flattened appearance. The galaxy exhibits a concentrated central bulge, which appears brighter and more densely packed than its outer regions. The color profile indicates a dominance of older stellar populations, suggesting lower levels of current star formation. There are no prominent spiral arms or significant dust lanes visible. Minor asymmetries and irregularities in the outer regions suggest past or ongoing interactions, though no major merging event is immediately apparent. Overall, the galaxy appears to be a moderately massive system, likely a disk galaxy viewed at a high inclination angle, or a galaxy transitioning from a spiral to an elliptical morphology.
