The galaxy exhibits an elliptical morphology, with a smooth, centralized concentration of light. The central region displays a yellowish hue, possibly indicative of an older stellar population. Progressing outward from the center, a gradual transition to a bluer color is observed, suggesting the presence of younger stars in the outer regions. The galaxy’s shape appears to be somewhat elongated, exhibiting a cigar-like form. There are no prominent features such as spiral arms or a distinct disk. No signs of major galactic mergers or significant tidal disturbances are apparent.
