The galaxy presents as a centrally concentrated object with a relatively smooth, featureless morphology. Its overall shape appears roughly elliptical, exhibiting a soft, gradual decline in brightness from its core to the outer regions. The color profile is dominated by bluer hues, most pronounced near the center, suggesting the presence of a younger stellar population and ongoing star formation activity. There is a subtle elongation, hinting that the object is not perfectly spherical, but rather a somewhat flattened spheroid. No distinct spiral arms or prominent dust lanes are discernible within this image resolution. There might be a subtle distortion in the outer halo, suggesting potential minor gravitational interaction or disturbance.
