The galaxy presents as a moderately luminous, disk-shaped object with an estimated redshift of approximately 0.23. Its morphology appears largely smooth, with a slight elongation suggesting an intermediate shape between round and cigar-shaped. There is a faint, discernible disk-like structure, though the overall appearance is dominated by a relatively featureless distribution of light. No major signs of ongoing or recent merger activity are evident. The color profile suggests a population of older stars. The star formation rate is low and the specific star formation rate is very low. 
