The galaxy presents as a relatively smooth, elliptical-like structure. The central region exhibits a concentration of yellow-white light, indicative of an older stellar population. Moving outwards from the core, the color shifts slightly to a more yellow hue before fading out into the blackness of space. A faint, disturbed feature appears at one end of the galaxy, possibly caused by a minor gravitational interaction. There are no clear indications of prominent spiral arms or significant dust lanes; the overall morphology suggests a galaxy that has largely exhausted its gas reserves or has undergone a significant merging event in the past that has disrupted any pre-existing spiral structure. The light distribution is highly concentrated, suggesting a relatively high mass. The size appears moderately compact.
