This galaxy presents as a disk galaxy, viewed nearly edge-on. A prominent central bulge is evident, exhibiting a smooth, concentrated light profile. The bulge appears yellowish-orange in color, suggesting an older stellar population. A disk structure surrounds the bulge, showing a bluer hue, potentially indicative of ongoing star formation. The disk appears relatively smooth, with little evidence of distinct spiral arm structures. The galaxy possesses a moderate redshift and estimated to be of substantial mass. Star formation rate is expected to be fairly low. Based on the angle of observation and the apparent flatness of the disk, it is likely a late-type spiral galaxy. No signs of any merging activity are present.
