The galaxy appears as a moderately inclined disk, with an elliptical morphology. Its central region exhibits a bright, concentrated bulge, suggesting a significant population of older stars. The galaxy's disk is relatively smooth, without prominent spiral arm structures visible in this image. A subtle color gradient is present, with the bulge showing a slightly redder hue compared to the bluer disk, possibly indicating ongoing star formation in the outer regions. There is a slight hint of a disturbance in the disk, potentially due to a minor interaction or merger event in its past. The galaxy lacks any strong tidal features.
