The galaxy presents a generally smooth and elliptical morphology, lacking prominent spiral arms or a well-defined disk structure. The central bulge is fairly luminous, exhibiting a concentrated brightness gradient towards the core. The overall color appears slightly redder, indicative of an older stellar population, with subtle variations in hue suggesting possible regions of differing stellar ages or dust content. There are no obvious signs of active galactic nuclei activity or prominent star-forming regions visible within the image. The edges of the galaxy gradually fade out. There is very little to no evidence of any ongoing merger activity or tidal disturbances. The galaxy is of intermediate size.
