The galaxy appears relatively small and faint, exhibiting a predominantly smooth morphology. Its overall shape is somewhat elliptical, leaning towards an "in-between" classification rather than distinctly round or elongated. There is little indication of spiral arms or significant disk structures within the observed light. The color profile is dominated by bluer wavelengths, with slight tinges of green, suggesting ongoing star formation activity, although likely at a low rate. No signs of major mergers or significant tidal disturbances are visible. The galaxy appears to be a relatively undisturbed system, potentially a low-mass galaxy with modest star formation.
