The galaxy presents as a generally smooth and elliptical structure, with a high degree of central concentration. The color is predominantly yellowish-orange, with hints of redder hues, suggesting an older stellar population and potentially a lower rate of ongoing star formation. No distinct spiral arms or prominent dust lanes are discernible. There appears to be a subtle elongation or deviation from perfect circularity, hinting at a possible cigar shape. No strong evidence of major mergers or significant tidal disturbances is immediately apparent, although there could be minor distortions present. The light appears evenly distributed, with the majority concentrated towards the center.
