The galaxy presents as an elliptical morphology with a smooth, centrally concentrated luminosity profile. The core exhibits a yellowish hue, suggesting an older stellar population. The outer regions are less luminous and display a bluer color, possibly indicating the presence of younger stars but in lower quantities. The galaxy does not show evidence of a prominent disk structure or spiral arms. Its shape is noticeably elongated, appearing somewhere between rounded and cigar-shaped. There are no visible signs of major mergers or significant tidal disturbances in the immediate vicinity. The galaxy appears to be an isolated system with a moderate degree of star formation.
