The galaxy exhibits a primarily smooth morphology with a slight central concentration of light. There is a hint of a possible disk structure although it is not well-defined, showing a slight elongation of the central light distribution. The color profile suggests the presence of both older stellar populations, indicated by reddish hues, and potentially some ongoing star formation, evidenced by the bluer regions in the galaxy's central area. There is also an indication of possible tidal features or disturbances. Although these do not suggest a major merging event, there is an asymmetry in the galaxy's light distribution with a faint extension or plume-like feature appearing. Overall, the galaxy appears to be in a relatively quiescent state but may have experienced a minor interaction or disturbance at some point in its past.
