The galaxy presents as a single, concentrated object with a generally smooth morphology. The light profile suggests a spheroidal shape, appearing nearly circular in projection. The central region exhibits a bright, concentrated core that gradually decreases in intensity towards the outer regions. A faint, diffuse halo surrounds the central bulge. Color gradients are subtle, but a slight bluer hue is observed in the immediate vicinity of the core. No distinct spiral arm structures, dust lanes, or other features indicative of disk galaxies are discernible. The overall appearance suggests a quiescent, relatively evolved system, without any significant signs of ongoing major star formation. There appears to be little to no evidence of recent or ongoing merger activity or tidal disturbances.
