The galaxy presents as a relatively smooth, centrally concentrated object. It appears nearly round, exhibiting minimal elongation or asymmetry. The galaxy's core is bright and compact, suggesting a high density of stars in the central region. A diffuse halo surrounds the core, gradually fading into the background. The color gradient indicates a potential difference in stellar populations, with bluer hues towards the central regions, suggestive of more recent star formation activity. The outskirts are redder, implying older stellar populations. There is no clear evidence of spiral arms, bars, or prominent dust lanes. Overall, the galaxy appears to be a relatively undisturbed system, showing no signs of major mergers or tidal interactions.
