The galaxy presents as an elliptical morphology, exhibiting a smooth, diffuse light distribution with minimal discernible internal structure. The luminosity profile increases gradually towards the center, culminating in a bright, moderately concentrated core.  The galaxy's shape appears somewhat elongated, deviating slightly from a perfect sphere. There is no apparent dust lane, spiral arm structure, or tidal tail, suggesting a lack of recent major merger events. The color profile shifts from yellowish-white towards the core to a bluer hue in the outer regions. The slight bluing could indicate a younger stellar population in the outer regions compared to the older, redder stars concentrated in the core. Faint, disturbed structures may be present in the surrounding area, potentially signifying ongoing minor interactions, though this could also be an artifact of data processing.
