The galaxy appears as a relatively smooth, elliptical structure with a concentrated central bulge. It exhibits a yellowish hue, suggesting an older stellar population. There is little evidence of spiral arms or significant dust lanes within the visible spectrum. The overall morphology indicates that the galaxy is likely a mature system, possibly undergoing relatively low levels of star formation. The light is fairly symmetrical, suggesting the galaxy is not undergoing a major merger, although subtle disturbances might be present upon closer inspection. Its shape is somewhat elongated, but significantly deviates from a cigar shaped structure, suggesting an intermediate ellipticity.
