The galaxy presents a generally smooth and elliptical appearance, with a high degree of central concentration. The core exhibits a bright, yellowish hue. The isophotes are largely regular, showing a slight deviation from perfect circularity towards an intermediate elliptical shape. There is very little evidence of spiral arm structure or distinct features such as dust lanes. There is a subtle indication of a minor disturbance in the outer regions of the galaxy, with a slight asymmetry to the overall structure. The overall color profile indicates relatively low levels of recent star formation, with a predominantly older stellar population. The size of the galaxy is rather moderate in extent.
