The galaxy appears as a moderately luminous, elongated object. It has a smooth and featureless appearance, with no distinct spiral arms or bar structure visible in this image. The light distribution suggests a centrally concentrated spheroid shape, possibly elliptical. There is a subtle color gradient, with the central region potentially exhibiting a slightly yellower hue, possibly indicative of an older stellar population. The outer regions appear bluer, suggesting the presence of some younger stars, although overall the galaxy appears quiescent in terms of star formation activity. The high cigar-shaped fraction suggests that it is highly elongated. There are no signs of any major mergers or disturbances.
