The galaxy presents a largely smooth, elliptical morphology. It exhibits a bright, concentrated central bulge that graduates outward to a less defined halo. The galaxy's color profile suggests an older stellar population, with a general red-yellow hue. There is no apparent disk structure, spiral arms, or significant dust lanes visible within the limitations of the image resolution. The galaxy's overall shape is generally round. There's no obvious sign of ongoing major merger events or tidal disturbances, although subtle irregularities could be present that are not visible in this image. The light distribution implies a centrally concentrated mass distribution. Star formation appears to be minimal.
