The galaxy presents a morphology consistent with a relatively smooth, elliptical system. The core is bright and concentrated, appearing a pale orange hue, which may indicate an older stellar population dominating the central region. Surrounding the core is a less intense, more diffuse halo exhibiting a slightly greenish-yellow tint. This may suggest the presence of a younger, albeit diminishing, stellar population and some ongoing, though limited, star formation activity. The overall shape is generally ellipsoidal but notably deviates from being perfectly round, exhibiting a slight elongation. No distinct spiral arms or significant dust lanes are visible. There is no clear evidence of any major ongoing merger events, though the galaxy's form implies some potential interaction history. Overall, the galaxy appears to be a massive system, generally evolving towards quiescence.
