The galaxy presents as an elliptical morphology, appearing largely smooth with no distinct spiral arm structures or prominent dust lanes visible. The object exhibits a concentrated central bulge, which displays a yellowish hue, potentially indicating an older stellar population. Moving outwards from the core, the galaxy's luminosity gradually diminishes, creating a diffuse halo that blends with the surrounding background. The galaxy appears elongated, deviating from a perfect spherical shape. There is no evidence of tidal tails or significant disturbances in its structure, suggesting it is not currently undergoing a major merger event. The overall color profile implies a low rate of ongoing star formation.
