The galaxy presents as a relatively smooth, elliptical structure with a noticeable central bulge that is brighter and more concentrated in luminosity. Its overall shape is elongated, appearing cigar-shaped, with no prominent spiral arm structures or distinct features that would indicate a disk galaxy. The color profile suggests a population of older stars, with a yellowish hue dominating the central regions. The edges of the galaxy appear more diffuse, fading gradually into the background sky, possibly indicating a sparse halo or envelope of stars surrounding the main body. There is no apparent evidence of ongoing major merging events or tidal disturbances; the overall structure appears relatively undisturbed.
