The galaxy appears to be a relatively smooth, elliptical or lenticular type. It displays a centrally concentrated luminosity profile, with a bright, well-defined core. There is no strong evidence of spiral arm structure or a prominent disk. The galaxy's color suggests an older stellar population, with a yellowish hue indicating the presence of evolved stars. Faint, somewhat diffuse, blueish regions are asymmetrically distributed in the outer regions. The galaxy exhibits a slightly elongated shape, but is generally rounded. There appear to be slight signs of disturbance within the galaxy itself. Overall, the galaxy appears to be a mature, relatively quiescent system undergoing low levels of star formation.
