The galaxy presents a generally smooth morphology, appearing elliptical in shape. The central region is highly luminous, exhibiting a bright, concentrated core. The luminosity appears to decrease steadily from the center towards the outer edges of the galaxy, without a clear disk structure. The colour profile suggests a relatively evolved stellar population, with a redder hue dominating the central bulge. There are no obvious signs of spiral arms or significant dust lanes. A slight asymmetry may be present in the outer regions, but it is difficult to determine if it is a result of a minor interaction or internal processes. Overall, the galaxy appears to be an elliptical system, with an estimated stellar mass in the range of 10^10 solar masses. Current star formation appears to be low, with an implied specific star formation rate of around 10^-10 per year.
