The galaxy presents a largely smooth, elliptical morphology. Its core exhibits a bright, concentrated intensity, indicative of a substantial stellar population. Moving outwards from the core, the luminosity gradually decreases with no distinct spiral arm features observed. The color profile reveals a yellowish-red hue, suggesting an older stellar population with a lower rate of active star formation, yet also a blue component suggesting the galaxy does have some star formation. The overall appearance suggests that it is a relatively massive system, though the slight deviation from a perfect elliptical shape could hint at a prior minor interaction or disturbance.
