The galaxy presents as a somewhat elongated, lenticular-like structure. It displays a smooth, largely featureless morphology, lacking any distinct spiral arms or prominent dust lanes. The light distribution appears centrally concentrated, exhibiting a gradual decline in brightness from the core outwards. The color gradient suggests an older stellar population, with a yellowish hue dominating the galaxy's overall appearance. There is no clear evidence of ongoing major star formation activity within the visible extent of the galaxy. Minor disturbances are potentially visible, but it is difficult to tell.
