The galaxy presents as a centrally concentrated object with a relatively smooth overall appearance. There's a high degree of central luminosity, suggesting a prominent bulge component. The galaxy appears moderately elliptical, trending toward a cigar shape. There is no obvious presence of spiral arm structure or significant dust lanes in the image. The light distribution is fairly uniform and diffuse beyond the bright core, potentially indicating an older stellar population or a lack of significant recent star formation. There may be minor irregularities or faint tidal features suggestive of a past interaction, but on the whole the image does not indicate an ongoing major merger event.
