The galaxy presents as a relatively smooth and centrally concentrated object, with a likely elliptical morphology. Its color appears to be a pale blue, indicating the presence of a moderate population of younger, hotter stars, although the color is not overwhelmingly blue, suggesting a significant population of older, redder stars as well. The galaxy exhibits an elongated, but not extremely flattened, shape. There is no strong evidence of significant spiral arm structure or a prominent disk component. Minor disturbances may be occurring, as the structure is not perfectly smooth, hinting at potential minor gravitational interactions, but the galaxy overall appears relatively undisturbed. The galaxy's size is relatively compact; it appears to be a dwarf galaxy, which is confirmed by the relatively low mass. The low SFR (star formation rate) also suggests the blue tint is more likely from a population of older stars, and that the galaxy is largely quiescent, with only a low level of ongoing star formation.
