The object in question appears to be a relatively smooth, elliptical galaxy. It exhibits a high degree of central concentration, with light gradually diminishing towards the outer edges. The galaxy possesses a slightly yellowish hue, suggestive of an older stellar population and reduced ongoing star formation. There's no obvious dust lane visible, nor any sign of spiral arms or significant irregularities in its structure. The galaxy’s round appearance indicates that it is likely viewed from a perspective close to face-on. A small number of what might be slight disturbances may be visible. Overall, this galaxy appears to be a typical example of a quiescent, early-type system.
