The galaxy presents as an elliptical morphology, highly elongated with an estimated physical radius of approximately 4 kpc. Its light profile appears smooth, indicating a dominant stellar population of older stars. The color index, derived from g, r, and z bands, suggests a redder, more evolved stellar population, consistent with low ongoing star formation. No clear signs of spiral arms or distinct features such as dust lanes are visible, which further supports its classification as an elliptical galaxy. There is a high probability this galaxy is not currently experiencing any major merging activity.
