The galaxy presents a predominantly smooth morphology. The overall shape is elliptical, appearing neither perfectly round nor highly elongated. There is a central concentration of light, possibly indicating a bulge. The color gradient suggests an older stellar population, trending towards redder hues in the central regions. Faint, diffuse extensions are potentially present, though indistinct, and the galaxy does not show obvious signs of spiral arms or significant dust lanes. No merging or tidal features are immediately apparent, though there is a slight irregularity that suggests minor interactions. Overall, the galaxy appears to be a relatively evolved system.
