The galaxy presents a generally smooth morphology, with a dominant, centrally concentrated bulge. The light distribution appears relatively symmetric, lacking prominent spiral arms or distinct features associated with active star formation in the disk. The galaxy exhibits an overall elliptical shape, appearing moderately rounded, rather than highly flattened or elongated. There is no strong evidence of tidal tails, bridges, or other significant disturbances indicative of a recent major merger event, although some minor asymmetry in the outer regions is visible. The color profile suggests an older stellar population with little to no ongoing star formation.
