The galaxy presents as a smooth, elliptical morphology. It exhibits a concentrated central bulge with a radial decrease in luminosity towards the outer regions. The galaxy appears to be largely featureless, lacking prominent spiral arms or a distinct disk structure. There is some evidence of minor irregularities or disturbances within the galaxy's structure. The galaxy displays a color gradient, with the central regions appearing more yellowish, potentially indicative of an older stellar population. Outer regions exhibit bluer hues which suggests ongoing, but not significant, star formation. The galaxy does not appear to be undergoing a major merging event, however there are some minor disturbance in the outer regions. The roundness falls somewhere in between round and cigar shaped, but looks more close to round.
