The galaxy appears as a moderately luminous object with a generally smooth morphology, although subtle features suggest some form of disturbance or interaction may be occurring. The shape is somewhat elongated, trending towards a flattened, oblate spheroid. The central region exhibits a concentration of yellowish light, potentially indicating an older stellar population or dust obscuration. Fainter, bluer light extends outward from this central region, suggesting the presence of younger stars and potentially ongoing star formation. No strong spiral arms or a well-defined disk are apparent, but there is evidence of some disky structure. The object seems to be undergoing, or has recently undergone, some form of interaction or minor disturbance. Overall, the galaxy presents characteristics of an intermediate-type system, possibly between a spiral and an elliptical.
