The galaxy presents as a moderately-sized, slightly elongated structure. It is characterized by a relatively smooth, diffuse light distribution, though some substructure hints at a possible disk component. Its color indices suggest a redder overall population, indicative of an older stellar population and lower levels of recent star formation. There is a notable absence of prominent spiral arms or other significant morphological features. Visual inspection suggests the galaxy is not undergoing any major merging events, though minor disturbances cannot be ruled out. Overall, the galaxy appears to be an intermediate type, potentially a late-type spiral or an early-type lenticular.
