This galaxy presents as an elliptical structure, exhibiting a generally smooth morphology with a concentrated central bulge. The light distribution is more intense towards the core, decreasing gradually outwards with no prominent spiral arm features. Color gradients are subtle, but there appears to be a slight reddening towards the center, which might indicate an older stellar population within the galactic nucleus, or a greater presence of dust. Overall, there is not significant evidence of recent major merger activity, although some faint asymmetries in the outer regions cannot be ruled out as signs of minor disturbances.
