The galaxy presents as an elliptical type, exhibiting a generally smooth and concentrated morphology. The central region shows a significant concentration of light, appearing a warm yellow hue, suggesting a population of older stars. There is some evidence of a slight extension, giving it a somewhat rounded appearance, it does not appear perfectly spherical. No distinct spiral arms or prominent dust lanes are visible. The galaxy's color profile leans toward the redder end of the spectrum, with the more distant outer regions exhibiting a less intense glow. There is a lack of any distinct features of active star formation, such as blue knots or HII regions. Any evidence of an ongoing or recent merger is generally not evident in the image. It appears to be a relatively undisturbed, relaxed system.
