The galaxy appears to be a disk galaxy viewed at a high inclination, possibly an edge-on orientation. The central bulge is prominent, exhibiting a relatively smooth, concentrated light distribution, with a slight yellowish hue. The disk component, extending laterally from the bulge, shows a bluer tint, suggestive of ongoing star formation, though the resolution is not sufficient to resolve individual star-forming regions or dust lanes. The galaxy does not exhibit any strong visual evidence of major mergers or significant tidal disturbances. Its general form indicates that is likely a non-interacting, relatively isolated system that is in the process of slowly forming stars.

The dimensions of the galaxy suggest that it is a medium-sized object, with the majority of the light contained within a radius of approximately 5 kpc. Overall, the galaxy appears to be a well-ordered system.
