The galaxy presents as an elliptical morphology, appearing generally smooth with a high degree of central concentration. The light distribution suggests a relatively homogeneous stellar population. The galaxy exhibits a slight elongation, with a moderate ellipticity. The color profile is predominantly red-yellow, indicative of an older stellar population and reduced star formation activity. There is no evidence of spiral arms, a central bar, or significant dust lanes. The overall appearance suggests a mature system. There may be a faint, diffuse halo surrounding the primary galactic body.
