The galaxy presents as a luminous object with a centrally concentrated morphology. The core exhibits a bright, yellowish hue, suggestive of an older stellar population. Moving outwards from the core, a subtle disk component is perceptible, displaying hints of bluer colors, potentially indicative of ongoing star formation. The overall shape appears to be somewhat flattened but largely elliptical. There are subtle irregularities within the galactic structure. These irregularities potentially indicate minor gravitational interactions or disturbances within the recent history of this galaxy.
