The galaxy presents as a largely elliptical structure, with a high degree of central concentration. The core region exhibits a bright, diffuse glow, transitioning outwards into a less luminous halo. The morphology suggests a relatively smooth, featureless distribution of light, with no readily apparent spiral arms or prominent dust lanes. The shape appears generally round, with only a slight elongation, potentially indicating a minor degree of rotational support. The color profile exhibits a redder hue in the central regions, gradually shifting towards bluer tones in the outer regions. This color gradient could be indicative of an older stellar population dominating the core, with younger, bluer stars contributing more significantly to the light in the extended halo. The overall appearance suggests a relatively evolved system, possibly an early-type galaxy with a suppressed star formation rate. There are hints of possible minor disturbances in the outer edges that may suggest previous or current gravitational interactions.
