The galaxy presents as a somewhat elliptical, though not perfectly round, structure. Its core is distinctly bright and concentrated, indicative of a significant stellar population and potentially an active galactic nucleus. The color profile suggests a primarily older stellar population, exhibiting a reddish-gold hue in the outer regions. There is a hint of blue around the central bulge, which may indicate a bit of star formation here. The overall texture is relatively smooth, lacking strong evidence of spiral arms or prominent dust lanes, though there may be some minor disturbances and possible ongoing merger activity.
