The galaxy presents as a relatively compact object. It appears as a smooth, centrally concentrated mass. The shape is somewhat elliptical, appearing more in between round and cigar shaped. There might be a hint of minor disturbance in its structure, but the dominant impression is one of relative uniformity. The light profile appears generally smooth. Color analysis reveals slightly higher luminosity in bluer bands, suggesting possible ongoing star formation, although the overall color seems skewed towards a redder spectrum, hinting at an older stellar population. There appears to be no obvious spiral arm structures or significant dust lanes visible.
