The galaxy presents a largely smooth, elliptical morphology with a central concentration of light that gradually diminishes outwards. There is a faint suggestion of a disk component, but this is not clearly defined and is heavily subordinate to the dominant spheroidal shape. The galaxy exhibits a relatively uniform color profile, with a redder hue overall, indicative of an older stellar population and potentially lower levels of current star formation. There does not appear to be any ongoing major merger events, although a minor asymmetry or distortion cannot be entirely ruled out. The galaxy appears to be relatively isolated in the field, without any obvious signs of strong tidal interactions with nearby companions.
