This galaxy exhibits a clear disk-like morphology, viewed nearly edge-on from our line of sight. A central bulge is present, appearing somewhat rounded in form. The galaxy's light profile suggests an older stellar population, with a distinct yellow-orange hue. There is no readily apparent evidence of active galactic nuclei or major merging events. Faint structures within the disk region are discernable, which could potentially indicate the presence of dust lanes or faint spiral arm fragments, though higher resolution imaging would be necessary to confirm. The overall smooth appearance of the disk implies that there are not strong star forming regions, although ongoing star formation activity is suggested by the observed colors.
