The galaxy presents a generally smooth morphology, with a noticeable central concentration. The overall shape appears largely elliptical or spheroidal rather than a well-defined spiral structure. There is some evidence of subtle features or irregularities that disrupt the smoothness, perhaps a hint of a disk but they are not prominent. The galaxy exhibits a relatively round appearance with a slightly elongated shape. There is no strong indication of ongoing or recent major mergers, nor are there any tidal tails or strongly distorted features indicative of strong gravitational interactions. There is a hint of a potential minor disturbance, but is not highly pronounced. The color profile suggests a moderately evolved stellar population. The overall color seems to be somewhat red. 
