The galaxy presents as a slightly elliptical structure with a bright, concentrated central bulge. The bulge exhibits a yellowish-white hue, suggestive of an older stellar population. Fainter, bluer regions are observed within the surrounding disc, indicating ongoing star formation. There are faint signs of spiral arm structures emanating from the central region, though they are not well-defined. The galaxy exhibits a moderate amount of internal structure, with some suggestion of disturbances or irregularities in its morphology.
