The galaxy presents an overall elliptical morphology, appearing smooth and relatively featureless. It exhibits a concentrated central bulge that gradually diffuses outwards into a fainter halo. The galaxy's shape is elongated, with an intermediate ellipticity, but not cigar-shaped. There is no visible evidence of a prominent disk structure or spiral arms. The galaxy's color profile suggests a relatively homogenous stellar population, leaning towards older, redder stars, particularly within the central bulge. There are no visible signs of ongoing major merging activity or significant tidal disturbances. Minor disturbances may be present but are not definitive from this image.
