The galaxy presents as a somewhat diffuse object, exhibiting an overall elliptical morphology. The light distribution appears relatively smooth, with a concentration of luminosity towards the central region. There is a subtle elongation visible along one axis, suggesting a degree of flattening. The color profile indicates a generally reddish hue, with hints of localized, brighter yellowish concentrations within the galaxy's structure. These areas could potentially represent regions of active star formation, though their definitive nature would require further spectroscopic analysis. There is no obvious indication of a prominent disk structure or spiral arms, nor are there any easily discernable tidal features or signs of recent major mergers. The galaxy appears relatively undisturbed.
