The galaxy presents a generally smooth, elliptical morphology, with a relatively high degree of central concentration. The light profile appears consistent with an early-type galaxy, exhibiting a fairly symmetrical and well-defined structure. The core region displays a yellowish hue, suggesting an older stellar population. The absence of prominent spiral arms or significant dust lanes implies a lack of active star formation. Faint disturbances can be seen at the outer edges of the galaxy, it is slightly asymetrical. The galaxy has some features that suggest a lack of recent merger, but might have undergone one in the past.
