The galaxy presents a primarily smooth morphology. The shape appears somewhat elliptical, deviating slightly from a perfectly circular form. The central region exhibits a bright, concentrated core. This core is surrounded by a fainter, more diffuse halo of light. A hint of a disk-like structure is observed, oriented nearly edge-on with respect to our line of sight, indicated by a slight flattening. There are no prominent spiral arms. Faint, disturbed-like light can be seen around the central core. There appears to be a slight indication of a possible minor interaction or disturbance within the galaxy's structure, although it's not a clear merging event. The general color is suggestive of an older stellar population.
