The galaxy appears to be a relatively smooth, elliptical-like system. It exhibits a bright, concentrated central bulge which dominates the overall light profile. Moving outward from the core, the light intensity decreases gradually, suggesting a fairly uniform stellar distribution within the galaxy's main body. The galaxy's color profile indicates a yellow-red hue across its entirety, which indicates an older stellar population with suppressed star formation. There may be a slight disk structure, but this is difficult to confirm without additional data. There are no obvious signs of recent mergers or major disturbances in the galaxy's morphology, though there are possible irregular features that suggest a potential minor interaction. Overall, the galaxy presents as a typical elliptical galaxy at intermediate redshift, with a well-defined structure and a lack of prominent star-forming regions.
