The galaxy presents as a generally smooth and elliptical object. It is elongated in shape, exhibiting a cigar-like morphology rather than appearing perfectly round. The color gradient shows a concentration of yellowish-orange light towards the center, suggesting an older stellar population dominates the core. Fainter bluish light is marginally observed in the outer regions, indicating a possible small population of younger, hotter stars or some degree of ongoing, albeit subdued, star formation. There is no obvious presence of spiral arms, bars, or significant dust lanes. No signs of major mergers are apparent, though a subtle asymmetry might suggest a minor gravitational interaction or disturbance in its past. Overall, the galaxy appears as a relatively evolved and quiescent system.
