The galaxy presents a generally smooth, elliptical morphology, with a noticeable elongation along a primary axis. The central region exhibits a bright, concentrated core that appears yellowish-orange, suggesting an older stellar population dominating this area. Surrounding the core is a more diffuse halo, transitioning to bluish hues in the outer regions. This color gradient indicates a possible shift towards younger, bluer stars in the galaxy's periphery. The overall structure appears relatively undisturbed, lacking prominent spiral arms or signs of recent major mergers, although subtle irregularities in the outer halo may point to minor gravitational interactions or past accretion events. The galaxy's shape is distinctly cigar shaped. The galaxy exhibits a substantial mass, with a moderate rate of star formation.
