The galaxy presents as a relatively smooth, concentrated object. It exhibits a generally elliptical morphology, tending towards round but with some slight elongation. The color profile is dominated by warmer tones, with a central bright region exhibiting a yellow-orange hue, suggestive of an older stellar population. The outer regions of the galaxy appear fainter and exhibit a subtle shift towards redder colors, which might be due to dust obscuration or differing stellar populations. There is no obvious evidence of spiral arms or significant dust lanes visible in this image. No significant tidal features or signs of recent major merger activity are immediately apparent. Overall, the galaxy appears to be a relatively quiescent system.
