The galaxy presents a smooth, elliptical morphology. It is centrally concentrated, exhibiting a bright, diffuse core that gradually fades into the outer regions. The overall shape is predominantly round, with a slight elongation suggestive of a cigar shape. There's a subtle asymmetry in the outer regions, with a faint hint of a disturbance. The galaxy appears generally isolated, with no prominent signs of ongoing major merging activity. The color profile indicates a redder hue, characteristic of an older stellar population. No distinct spiral arms or prominent dust lanes are discernible within the galaxy's structure.
