The galaxy presents as a moderately bright, elliptical structure with a smooth, diffused appearance. It has an intermediate ellipticity, appearing neither perfectly round nor elongated into a cigar shape. A central bulge region is visible, exhibiting higher luminosity compared to the outer regions of the galaxy. This suggests a concentration of older stellar populations towards the galaxy's core. There's no clear evidence of spiral arm structure or significant dust lanes. The galaxy displays a relatively uniform color profile, hinting at a lack of recent major star formation activity across the galaxy and instead dominated by older stars. There may be some ongoing, low level star formation activity present, but nothing that significantly distorts the smooth, featureless light profile of the galaxy. The galaxy does not show any clear signs of major mergers or significant tidal disturbances.
