The galaxy presents as a centrally concentrated, somewhat elliptical object. A prominent, reddish core is visible, surrounded by a more diffuse, greenish halo. The overall appearance is relatively smooth, with no obvious spiral arm structures or dust lanes visible at this resolution. The light distribution suggests a dominant spheroidal component, and the galaxy does not appear to be undergoing any major mergers or significant tidal disturbances. The color gradient, from red in the center to green in the outskirts, may indicate a change in stellar populations, with older, redder stars concentrated in the core and younger, bluer stars further out, suggesting ongoing star formation. The galaxy's effective radius is estimated to be approximately 6 kpc, giving it an intermediate size. 
