The galaxy presents as a relatively smooth, elliptical-like structure, though not perfectly spherical. There may be a slight asymmetry or minor disturbance in the outer regions, but the overall form appears largely undisturbed. The central region exhibits a higher concentration of light, suggesting the presence of a prominent bulge or core. A smooth transition is observed from this central bright region towards the outer, fainter regions. The color profile appears relatively uniform across the galaxy, with a subtle shift towards redder hues in the central region. This may suggest an older stellar population concentrated toward the core with minimal ongoing star formation. The galaxy exhibits colors indicative of a relatively low star formation rate. The object is compact with a size of approximately 4 kpc.
