This galaxy exhibits a disk-like morphology, viewed at a significant angle, approaching edge-on. A central bulge is visible, exhibiting a yellowish-white hue, potentially indicative of an older stellar population. Fainter, bluer regions are present in the disk, possibly indicating areas of more recent star formation. Some patchy redder regions are also present. The galaxy does not show strong evidence of major mergers or significant tidal disturbances, though some minor asymmetries are apparent. Based on observed color indices, the galaxy presents a moderately luminous profile with an estimated stellar mass on the order of 10^11 solar masses. The rate of star formation appears to be relatively low.
