This galaxy appears to be an elliptical galaxy, exhibiting a generally smooth and concentrated light distribution. The core region presents a yellowish-white hue, suggesting an older stellar population dominated by red giant and main-sequence stars, with little ongoing star formation. The galaxy's radial profile indicates a gradual decrease in luminosity outward from the core. There is no discernable spiral arm structure or dust lanes. The shape appears roughly circular, with only a slight deviation towards an elongated form. There's no visual indication of any major merger activity, such as tidal tails or strong asymmetries, but some possible minor disturbances cannot be ruled out at this resolution. The overall morphology indicates a galaxy that has largely exhausted its gas reserves and is in a relatively quiescent phase of its evolution.
