The galaxy presents as a relatively smooth, elliptical morphology. The light distribution appears concentrated towards the center, with a bright, prominent bulge. There's a gradual fading in intensity from the core outward, suggesting a lack of distinct spiral arms or other defined structures. The overall shape is closer to round than elongated, but is still slightly elongated. There is no obvious evidence of an ongoing merger, although some minor asymmetry or faint tidal features cannot be completely ruled out due to the image resolution. The color appears to be relatively uniform across the galaxy, trending towards redder hues, which may indicate an older stellar population with lower recent star formation.
