The galaxy presents as a generally smooth object, exhibiting an elliptical morphology. It appears approximately circular, with a slight elongation along its major axis. The color profile indicates a dominant reddish-yellow hue, concentrated primarily in the central bulge region. This suggests a stellar population of older, redder stars. There is very little evidence of spiral arm structures or significant dust lanes within the galaxy, implying a lack of ongoing, high-rate star formation. There may be slight disturbances, but they are mostly symmetrical. Overall, the galaxy seems to be an evolved system with low star formation.
