The galaxy presents as a spiral type, displaying a prominent, moderately sized central bulge. This bulge exhibits a yellowish hue, suggesting an older stellar population. Extending from the central bulge are two clearly defined spiral arms, wound relatively tightly. These arms display a bluish tint, indicative of ongoing star formation. A strong bar structure appears to bisect the central bulge. The overall structure of the galaxy shows no evidence of significant tidal disruption or ongoing major merger activity. The galaxy is not seen edge-on, presenting a face-on aspect. There are no obvious signs of an active galactic nucleus in this image.
