The galaxy presents as an elongated object with an apparent cigar shape. The central region exhibits a higher concentration of light, appearing brighter and more yellow in color, possibly indicating an older stellar population. The outer regions appear fainter and more diffuse, with a hint of blue light suggestive of some ongoing star formation. There are no readily identifiable spiral arms or other distinct features. The galaxy appears relatively smooth, with no major disturbances or merging events immediately apparent. The galaxy exhibits a red shift of z~0.17 implying significant recession velocity. Considering the distance implied by the red shift, the galaxy is estimated to have a moderate size and mass. The rate of star formation is relatively low.
