The galaxy appears as a moderately luminous, elongated structure. Its overall morphology suggests an elliptical or lenticular classification, displaying a dominant, smooth component with some irregularities. The central region shows a concentration of light, potentially indicative of a galactic nucleus. The color profile suggests an older stellar population, exhibiting redder hues with a hint of yellow, especially within the central bulge. Fainter, bluer regions are sparsely scattered towards the edges of the galaxy, which could indicate younger stars or star forming regions. There is a possible disk-like structure that is not well defined. The overall visual impression implies a mature system with a relatively low star formation rate. There is also a subtle hint of disturbances within the main structure, which might point to a past or ongoing interaction with another galaxy.
