The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a high degree of central concentration, with a bright, prominent core region gradually fading outward. The light distribution suggests a spheroidal shape, with an approximate diameter of 2.4 kpc as seen from our vantage point. No obvious spiral arm structures or dust lanes are discernible within the resolution of the image. The color gradient transitions from a yellowish hue in the core to a slightly redder color in the outer regions, potentially indicating an older stellar population dominating throughout. There is a very slight flattening on one side of the galaxy's halo. This is possibly from a minor tidal interaction but could also be related to the conditions of its formation. Overall, the galaxy gives the visual impression of being relatively quiescent, lacking the hallmarks of ongoing, rapid star formation.
