The galaxy appears to be an elliptical type, characterized by a smooth, centrally concentrated light distribution. The central region exhibits a yellowish hue, suggestive of an older stellar population. Moving outward from the core, the color transitions to a slightly bluer shade, possibly indicating a small population of younger stars. Overall, the galaxy lacks any distinct features such as spiral arms or a prominent disk. There is no obvious evidence of ongoing major mergers, however, the shape of the galaxy is not perfectly spherical, so potentially there have been minor disturbances. The galaxy does not appear particularly active in terms of star formation.
