The galaxy presents as a single, centrally condensed object. Its overall morphology appears relatively smooth, with a dominant spheroid component. There is no obvious spiral arm structure or bar feature visible in the image. The galaxy exhibits a yellowish-orange hue, possibly indicating an older stellar population with fewer hot, young stars. There might be faint hints of some very minor disturbances in its disk but they are not pronounced. It would be beneficial to obtain spectroscopic data to confirm the nature of the galaxy's stellar population and further investigate its dynamics.
