The galaxy presents as an edge-on disk galaxy, exhibiting a notable degree of flattening. Its overall structure appears smooth. The central bulge is prominent and exhibits a relatively concentrated brightness profile, suggesting a high stellar density. Dust lanes are not readily apparent within the disk, potentially due to the viewing angle or a low dust content. The color profile suggests a higher concentration of older stellar populations, particularly within the bulge. The lack of clear spiral arm structure or prominent HII regions reinforces the impression of a relatively quiescent or passively evolving system. There is no evidence of strong tidal features or morphological disturbances, which indicates that a major merger event has not occurred. Overall, the galaxy exhibits an appearance consistent with a passively evolving disk galaxy viewed nearly edge-on.
