The galaxy appears as a centrally concentrated object, exhibiting a generally smooth morphology. Its light profile suggests a relatively even distribution of stars, lacking prominent spiral arms or a well-defined disk structure. The galaxy's color appears to be moderately redder, which suggests an older stellar population. There is no apparent ongoing major star formation, but there could be little to no minimal star formation still occurring. Given its round shape, it is likely an elliptical galaxy or potentially a lenticular galaxy viewed face-on. There's no evidence of significant tidal disturbances or mergers in progress, but there may be a very minor disturbance.
