The galaxy presents as a relatively smooth, elongated structure. It appears to be an elliptical galaxy seen edge-on, or a lenticular galaxy with a prominent bulge and a disk oriented along our line of sight. The central region exhibits a brighter, more concentrated luminosity, suggesting a higher stellar density. The disk component, if present, appears fainter, and smoothly transitions into the outer regions. There is little evidence of spiral arm structure or distinct dust lanes. The color profile suggests an older stellar population, with a slight bluer hue to the outer regions. There is no evidence of active galactic nuclei or ongoing major starburst activity. Possible signs of minor interaction with another galaxy.