The galaxy presents as a relatively smooth, elliptical-like structure with a centrally concentrated luminosity. It appears moderately elongated, exhibiting a shape somewhere between round and cigar-shaped. There is a lack of defined spiral arms or significant dust lanes within its structure. The galaxy's color profile suggests a redder overall hue. Based on the image alone, no signs of a major merger event or significant tidal disturbances are immediately apparent, though a subtle asymmetry might suggest minor gravitational interaction. The galaxy displays an absolute magnitude that indicates a relatively bright object. It is likely to be a massive galaxy with a modest rate of star formation.
