The galaxy appears to be a smooth, elliptical-type galaxy, displaying a high degree of central concentration. Its overall shape is elongated, exhibiting a cigar-like morphology. The core region presents a bright, yellowish hue, suggesting a population of older stars. Fainter, reddish tones are observed toward the outer regions of the galaxy, potentially indicating the presence of dust or a population of slightly younger stars. The galaxy does not show any obvious signs of spiral arms or ongoing major merger activity, although there could be minor disturbances due to past interactions. The light distribution within the galaxy appears relatively uniform, lacking any distinct features such as prominent star-forming regions.
