The galaxy presents an overall smooth morphology, appearing largely spheroidal in shape. The central region exhibits a high concentration of light, indicating a dense stellar population or an active galactic nucleus. This core is a yellow-orange hue, potentially indicative of an older stellar population. Fainter, bluer light extends outwards from this core, suggesting the possibility of ongoing, albeit subdued, star formation in the surrounding regions. Some minor asymmetric features are present, but there is no strong visual evidence of a major ongoing merger or significant tidal disturbance.
