The galaxy presents as a somewhat symmetrical, concentrated object. The core region exhibits a relatively smooth, amorphous structure, indicative of a significant spheroidal component. There's a subtle elongation or slight asymmetry, suggesting a possible interaction or internal dynamical process. The color profile appears reddish-yellow, implying a population of older stars, and possibly a small amount of dust obscuration. Overall, the galaxy seems to be reasonably evolved, potentially a transition type between spiral and elliptical. No clear spiral arm structure is apparent from this view.
