The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a moderately rounded shape, with some deviation towards an elliptical form. There may be a slight suggestion of a disk-like component, but it is not prominent.

There is no clear evidence of any major ongoing merger activity, although minor disturbances cannot be entirely ruled out. The galaxy's color profile appears to be redder, potentially indicating an older stellar population and/or a higher degree of dust obscuration. The galaxy has moderate mass and low levels of star formation.
