The galaxy presents as a smooth, elliptical form, exhibiting a concentrated central bulge. The light distribution suggests a relatively uniform stellar population, with a gradual decrease in luminosity moving outward from the core. The apparent elongation indicates a non-spherical shape, trending towards a cigar-like appearance. There is no clear evidence of spiral arms or significant dust lanes. The overall color profile leans toward the redder end of the spectrum, suggesting an older stellar population with relatively low current star formation. Minor disturbances cannot be entirely ruled out, but no major mergers are clearly evident from the observed morphology.
