The galaxy appears to be a relatively compact elliptical galaxy. Its light profile suggests a generally smooth distribution, lacking prominent spiral arms or a distinct disk. There might be a very subtle distortion of the overall elliptical shape, indicating a possible past or ongoing interaction, though a merging event is not readily apparent in this imagery. The color profile is fairly uniform across the galaxy. The apparent lack of significant blue light suggests a low star formation rate and a generally older stellar population. The object displays a somewhat rounded shape.
