The galaxy presents a primarily smooth morphology, with little apparent spiral structure. It appears to be elliptical in shape, with a high degree of central concentration. The core exhibits a notable luminosity, fading gradually into the outer regions of the galaxy. There appears to be a slight elongation to the galaxy's structure, suggesting it may be deviating from a perfect sphere, potentially transitioning towards a cigar shape. There is no sign of active merging or major disturbances. The galaxy seems to exist in isolation. In terms of color, it appears reddish-white overall, suggesting an older stellar population.
