The galaxy presents a primarily smooth morphology, exhibiting a central bulge that dominates its overall appearance. The bulge displays a yellow-orange hue, suggestive of an older stellar population. Moving outward from the bulge, there's a discernible disk component, though it is not sharply defined. The disk appears somewhat patchy in color distribution. A subtle greenish tint hints at the presence of ionized gas, potentially indicating ongoing star formation. The galaxy appears to be relatively isolated with no strong signs of tidal disruption or interaction with other galaxies. The galaxy's shape is intermediate between round and elongated.
