The galaxy appears as a single, fairly compact object with a generally smooth light distribution. The central region exhibits a somewhat round morphology, lacking prominent spiral arms or a strong bar structure. There might be a slight elongation or flattening to its overall shape, although this is not very prominent. There are no signs of any major mergers but there could be the hint of minor disturbances. The observed colors suggest a mix of stellar populations, with a dominant population of older stars contributing to the redder light, and a younger, bluer stellar population also present. Star formation rates appear low to moderate.
