The galaxy appears as a moderately bright, somewhat elliptical object. It presents a relatively smooth light distribution overall, with a central concentration of luminosity. Two distinct color components are observed within the galaxy's structure. The first, located in the apparent center, displays a warmer, yellowish-orange hue, potentially indicating a population of older stars or significant dust obscuration. The second component, slightly offset from the center, exhibits a cooler, bluish tint, possibly associated with regions of recent star formation or a population of younger, hotter stars. This color variation suggests the presence of distinct stellar populations and varying ages within the galaxy. There is some visual evidence suggesting minor asymmetry in the outer regions of the galaxy, possibly hinting at past interactions or disturbances, though no prominent tidal features or signs of an ongoing major merger are clearly visible.
