The galaxy presents as a relatively smooth, elongated structure with a noticeable color gradient. The central region exhibits a yellowish hue, suggesting a concentration of older stellar populations. Moving outward from the center, the color shifts towards a slightly redder tone. This may indicate a difference in stellar age or metallicity between the core and the outer regions. The galaxy's shape appears somewhat disturbed, possibly due to a past minor interaction or internal dynamics. There's a hint of asymmetry, although no clear spiral arms or distinct features are immediately discernible. The overall appearance is consistent with an elliptical or lenticular galaxy, exhibiting characteristics of a system where star formation is either low or has largely ceased. 
