The galaxy presents as a moderately bright, relatively compact object. Its overall color appears slightly reddish. Morphologically, it appears largely smooth, lacking prominent spiral arms or a distinct disk structure. There is a slight elongation, with the galaxy appearing somewhat cigar-shaped rather than perfectly spherical. Faint, subtle features are visible, hinting at a possible minor disturbance in its structure or perhaps the early stages of a weak interaction with a smaller object. There's no obvious evidence of a strong merger event, though subtle asymmetries cannot be ruled out. Based on the apparent color and smoothness, it may consist primarily of an older stellar population, though precise age determination requires spectroscopic data.
