The galaxy presents as a moderately inclined disk. A central bulge dominates the structure with a relatively smooth, concentrated light profile. The disk component shows some evidence of bluer star formation regions, although it is primarily composed of older stellar populations, given its redder color. Overall, the galaxy has an elliptical appearance, the bulge being relatively smooth. There are no visible signs of strong spiral arms. No signs of tidal disturbances or ongoing major mergers are apparent in this image. The galaxy appears to be fairly isolated.
