The galaxy presents an elliptical morphology, with a bright, concentrated central bulge. The light distribution within the galaxy appears relatively smooth and diffuse, transitioning from a highly luminous core to fainter, less defined outer regions. The overall shape deviates slightly from perfectly circular, exhibiting a slight elongation along a preferred axis. Color gradients are subtle, with a general trend towards bluer hues in the outer regions and redder hues towards the core. No distinct spiral arms or prominent dust lanes are discernible in this image. The lack of strong blue emission suggests a relatively quiescent star formation rate. The galaxy appears to be relatively isolated.
