The galaxy appears as a centrally concentrated object with a smooth, elongated morphology. The color distribution suggests a generally older stellar population, with a yellowish hue dominating the central region. There are subtle variations in color, possibly indicating differences in stellar population or dust distribution, but no distinct spiral arms or prominent star-forming regions are apparent. The overall light distribution is relatively even, suggesting a well-mixed stellar population. The shape is cigar-like, with an elongation along its major axis. There are no signs of major mergers or significant tidal disturbances. The object appears relatively undisturbed, consistent with a galaxy that has undergone significant morphological evolution.
