The galaxy presents as a relatively smooth, elongated structure. Its central region exhibits a concentration of light, appearing yellowish, suggesting an older stellar population. The outer regions show a faint bluish hue, hinting at the presence of younger, hotter stars and some ongoing star formation. The galaxy displays an elliptical morphology, with no discernible spiral arms or a prominent disk component. The overall appearance suggests that it is not currently undergoing any major mergers, although some minor disturbances may be present in its morphology. The galaxy is somewhat cigar shaped and appears generally smooth.