This galaxy exhibits a prominent central bulge, exhibiting a yellowish hue suggestive of an older stellar population. Fainter and less defined, bluish spiral arms extend from the central region into the surrounding disk. These arms indicate ongoing star formation. The overall shape is indicative of a disk galaxy, viewed at a slight angle relative to edge-on. The galaxy appears relatively smooth. There is no evidence of a strong bar structure. There are no indications of tidal tails or other obvious signs of a recent major merger event, though some minor disturbances cannot be entirely ruled out due to the image resolution.
