The galaxy appears as a relatively small, faint, and unresolved object. It presents a generally smooth, elliptical morphology, with a high degree of central concentration. There is little to no visible spiral arm structure or evidence of significant dust lanes. The color profile suggests a relatively older stellar population, indicative of a low star formation rate. The absence of distinct features implies a quiescent nature with minimal ongoing interactions or mergers. There is no clear presence of a bar or other strong structural components, just a relatively smooth, elliptical distribution of light.
