The galaxy presents as a generally smooth, elliptical object with a noticeable elongation along one axis, approximating a cigar shape. There is a concentrated central bulge exhibiting a high surface brightness, suggesting a significant stellar density in that region. The color profile indicates a dominant blue hue, which could imply the presence of a younger stellar population and ongoing star formation. No distinct spiral arm structures or dust lanes are readily apparent. The galaxy appears relatively undisturbed, lacking any obvious signs of major mergers or tidal interactions. The outer regions display a gradual fading in intensity, indicating a decreasing stellar density moving away from the galactic center.
