The galaxy presents as a relatively compact object. Its overall form appears largely smooth and elliptical, exhibiting a high degree of central concentration. There is a hint of a faint disk, but the dominant structure is spheroid-like. The core region exhibits a yellowish hue, potentially indicating an older stellar population. Surrounding the core is a more pronounced, greenish-blue envelope, suggesting ongoing star formation activity. The galaxy appears relatively isolated, without any obvious signs of major interactions or mergers, although a slight asymmetry might imply past tidal disturbance.
