The galaxy presents as a moderately sized, diffuse object, primarily red in coloration, suggesting a population of older stars and lower star formation rate. The morphology appears largely smooth, lacking any distinct spiral arm structures or a well-defined disk component. There is an indication of some irregularity in the galaxy's shape, which could be indicative of past or ongoing gravitational interactions. There is some concentrated light in the center of the object which is likely the bulge region. It has a faint blue coloration to the south and east of the bulge, indicating the potential presence of some star formation or a younger stellar population in that area. Overall, the galaxy appears to be an elliptical type or possibly a lenticular galaxy undergoing some minor disturbances.
