The galaxy presents a predominantly smooth morphology. Its form appears largely spheroidal, though not perfectly round, with a slight deviation from a circular shape. The light distribution is centrally concentrated, exhibiting a bright, relatively uniform core that fades gradually towards the outer regions. The color profile suggests an older stellar population; the central region displays a yellowish hue, likely indicating a greater abundance of evolved stars. There is no discernible spiral arm structure or significant dust lane obscuration visible within the resolution afforded by the image. A very minor disturbance is possible on the outer edges, but more data would be needed to confirm this. Overall, this appears to be a relatively isolated galaxy.
