The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge that appears largely featureless. The light profile appears to diminish steadily from the core outward, with no prominent spiral arm structures or dust lanes visible in this image. The overall shape tends towards round, exhibiting minimal elongation. There are no obvious signs of major mergers or significant tidal disturbances. Subtle irregularities or minor disturbances, if present, are below the detection threshold given the image resolution. The galaxy appears to have a somewhat uniform color gradient across its extent, suggesting a relatively homogeneous stellar population or a gradual shift in age or metallicity with radial distance from the center. There seems to be very little ongoing star formation, judging by the even blue hue and lack of brighter patches indicating star forming regions.
