The galaxy presents an overall elliptical morphology, appearing elongated along a major axis. The core exhibits a concentrated luminosity, suggestive of an older stellar population with a yellowish-orange hue. This central region smoothly transitions into a fainter, more diffuse halo. A subtle disk-like structure can be discerned along the galaxy's major axis. There is evidence of subtle disturbances in the galaxy's structure, possibly indicating a past or ongoing minor interaction. The bluer tint in its outer regions hints at more recent star formation than is present in the core. This galaxy displays only a moderate level of star formation activity and the image shows a substantial mass.
