This galaxy exhibits an elongated, cigar-like morphology. The central region displays a bright, concentrated core, indicating a high stellar density and potentially the presence of a supermassive black hole. The color profile suggests a significant population of older stars, with a yellowish hue dominating the core. Moving outwards from the core, the galaxy shows a gradual fading in brightness and a shift towards redder colors. A slight asymmetry in the outer regions, as well as blue spots, suggests minor disturbances. There are no clear signs of spiral arms or a well-defined disk structure. The overall smooth appearance, coupled with the elongated shape, could indicate that this is an elliptical galaxy, with potential evidence of a minor merger or tidal interaction influencing its shape.
