The galaxy presents as a slightly elongated, lenticular structure with a smooth appearance. The core region exhibits a yellowish hue, which may indicate an older stellar population. Moving outwards from the center, the intensity of the light diminishes gradually. There are hints of a faint disk-like structure, but the galaxy lacks any prominent spiral arms or significant dust lanes. There is no strong evidence of any ongoing major merger events or tidal disturbances, although there is a slight asymmetry in the light distribution. The color suggests that star formation activity is currently suppressed, resulting in a relatively red and dead galaxy.
