The galaxy presents as a relatively smooth, centrally concentrated object. The overall morphology appears elliptical, although a faint disk component cannot be entirely ruled out. There's a noticeable color gradient, with the core exhibiting a whiter hue that transitions to slightly bluer colors in the outer regions. No strong evidence of spiral arms or other distinct features is immediately apparent. There may be a very slight disturbance of the central core or a merging event. This is based on the central bulge, which is not completely round.
