The galaxy presents as a highly elongated, spindle-shaped object, suggesting an edge-on or near edge-on orientation relative to our line of sight. A distinct central bulge is apparent, exhibiting a yellowish-orange hue, which could indicate an older stellar population and a higher concentration of dust. The outer regions of the galaxy show a bluer color, suggesting the presence of younger, hotter stars and ongoing star formation. The light distribution appears relatively smooth, possibly indicating that the galaxy is an elliptical galaxy with an older, more settled stellar population. There may be evidence of a faint disk component but more data is needed to confirm. There are no obvious signs of recent major mergers or tidal interactions.
