The galaxy presents a relatively smooth and centrally concentrated morphology. Its overall shape appears elliptical, showing little evidence of spiral arms or a distinct disk structure. The light distribution suggests a predominantly older stellar population, with a color profile indicating lower levels of ongoing star formation. There are no obvious signs of tidal disturbances or mergers, suggesting a relatively quiescent evolutionary history. The galaxy exhibits a degree of roundness, deviating from a highly elongated or cigar-like form.
