The galaxy presents as a somewhat spheroidal object, appearing mostly smooth in texture. Its morphology does not obviously indicate the presence of spiral arms or a prominent disk structure. The light distribution suggests a central concentration of older stars, potentially with a relatively small ongoing star formation rate, or perhaps with star formation concentrated in a small region. There may be slight morphological disturbances within the galaxy, but it is difficult to determine if these are major, such as signs of a merger. The roundness is not very pronounced and is likely in between a round and cigar shape.