The galaxy presents an elliptical morphology, appearing largely smooth and featureless upon visual inspection. There's a high degree of central concentration with a gradual decline in luminosity outwards from the core, indicative of an older stellar population. The color profile suggests the presence of relatively little ongoing star formation, leaning towards the redder end of the spectrum. The overall shape appears close to round on the plane of the sky. There is no evident tidal debris or obvious signs of recent or ongoing major mergers, although a minor disturbance cannot be entirely ruled out based on the image resolution.
