The galaxy presents as a moderately luminous, relatively compact object. It appears to exhibit a smooth, elliptical morphology, with a high degree of central concentration. The color profile suggests a primarily older stellar population, with a yellow/red hue dominating the central regions. A slight elongation is visible, with some asymmetry. A faint disturbance in the galaxy's shape can be seen above the main body of the galaxy. There is little evidence of significant ongoing star formation based on the color profile.
