The galaxy appears to be a lenticular or possibly an elliptical galaxy, displaying a smooth, elongated morphology. The central bulge exhibits a yellowish hue, suggestive of an older stellar population. Progressing outward from the core, the galaxy transitions to a bluish color, potentially indicating the presence of younger stars. The overall shape is cigar-like, with no obvious spiral arm structures discernible. There are subtle irregularities along its edges, hinting at possible minor gravitational interactions with smaller satellite galaxies or past merger events. Overall, the galaxy presents a relatively quiescent appearance, lacking prominent signs of active star formation.
