The galaxy presents as a moderately bright, relatively compact object. Its morphology appears largely smooth, with a dominant, centrally concentrated bulge. Faint extensions emanate from the central region, though distinct spiral arm structures are not clearly discernible in this imagery. The galaxy exhibits a subtly elongated, somewhat rounded form. There are no obvious signs of ongoing major merging events or significant tidal disturbances, though minor asymmetries might be present. Color gradients are observed, with the central region appearing slightly redder than the outer regions, suggesting a difference in stellar populations or dust content. The galaxy's overall color index suggests it is neither exceptionally blue, indicating vigorous recent star formation, nor extremely red, indicating an old and passive stellar population. It seems to fall within an intermediate range, consistent with a relatively quiescent star formation rate.
