The galaxy appears to be an elliptical galaxy, characterized by a smooth, centrally concentrated light distribution. Its shape is roughly elliptical, with a slight elongation. There is no apparent disk structure or spiral arms visible, and the overall structure suggests a relatively old stellar population. The galaxy exhibits a central region that is bright in g, r, and z bands and has a yellow hue, with a magnitude such that star formation is present but minimal. The galaxy does not appear to be undergoing any major merging events or significant tidal disturbances. The absence of blue light suggests a lack of ongoing, significant star formation in the outer regions, consistent with a population dominated by older, redder stars.
