The galaxy presents a morphology consistent with a barred spiral type. Prominent spiral arms emanate from the central region, exhibiting a relatively open winding structure. The color gradients suggest a higher concentration of younger, bluer stars within the spiral arms.

The galaxy displays indications of a possible interaction or minor merger event. There appears to be a secondary structure or a disturbed region in proximity to the main galactic disk, potentially impacting the overall morphology.

The presence of strong bar features are suggested, a substantial fraction of the light appears to be concentrated in the bar. The estimated size suggests a moderate sized galaxy.
