The galaxy appears as an elliptical structure, exhibiting a smooth and concentrated morphology. The core is luminous with a yellowish hue, suggesting an older stellar population. Moving outwards from the center, the light gradually diminishes, with the outer regions displaying a bluer tint. The galaxy's overall shape is slightly elongated, but generally appears rounded. There is no clear evidence of spiral arms, bars, or significant dust lanes. The galaxy seems isolated and undisturbed, with no prominent signs of ongoing merger activity or tidal interactions.
