The galaxy presents as a moderately luminous, elongated structure. It is predominantly smooth in appearance, with a relatively featureless disk. The central bulge exhibits a yellowish hue, suggesting an older stellar population. The galaxy appears to be tilted significantly relative to our line of sight, presenting an edge-on or highly inclined perspective. There is a hint of bluer light towards the outer edges, possibly indicating some ongoing, albeit low, level of star formation. The galaxy does not show any obvious signs of major mergers or significant disturbances. Its color profile indicates it contains a mixture of both old and young stars, and its overall shape suggests that it is likely an elliptical galaxy.
