The galaxy presents a primarily smooth morphology, appearing elliptical in shape. A slight elongation is observed, deviating from a perfectly circular form. The central region exhibits a high concentration of light, indicative of a prominent galactic nucleus. The color profile suggests an older stellar population, with a dominant yellowish-red hue, particularly in the central bulge. Faint, diffuse extensions are visible, possibly representing tidal tails or remnants of past interactions, though these features are not pronounced. There is no clear evidence of spiral arm structure. Overall, the galaxy appears relatively undisturbed, with no signs of major merging events or significant star formation activity.
