The galaxy presents as a centrally concentrated object with a generally elliptical morphology. The core region exhibits a high degree of luminosity, appearing almost uniformly bright with a slightly yellowish hue. Moving outwards from the core, a disk-like structure is observed, though it lacks well-defined spiral arms. This disk displays a mottled appearance, with regions of faint blue interspersed with darker patches, suggesting the presence of both young, hot stars and dust lanes. The overall colour of the galaxy suggests a mature stellar population, with some ongoing, albeit limited, star formation in the disk. There is a slight disturbance to the shape of the galaxy, but the effects of this appear to be minimal, suggesting a stable structure.
