The galaxy presents as a relatively smooth, elliptical morphology. Its light profile exhibits a high degree of central concentration, with a bright core that gradually fades towards the outer regions. There is a distinct lack of any discernible spiral arm structure or prominent dust lanes. The color index suggests a population of older stars dominating the light output, with a redder hue compared to galaxies with active star formation. There may be evidence of very minor disturbances suggesting possible past interactions, but overall, the galaxy appears largely undisturbed. The shape is nearly round, with a smooth light distribution.
