The galaxy presents a diffuse, somewhat irregular morphology. It appears to be disc-shaped with a relatively bright, concentrated central bulge. Faint spiral arm structures might be present but are not well-defined in the image. The color distribution shows a bluer hue in the outer regions, possibly indicating ongoing star formation, while the central bulge exhibits a slightly yellower or whiter color, suggestive of an older stellar population. No significant tidal features or evidence of recent major merger activity are immediately apparent, although subtle disturbances cannot be ruled out. The galaxy's overall structure suggests a possible transition between a spiral and a lenticular type.
