The galaxy appears to be a disk galaxy, likely an elliptical, viewed at a significant angle relative to its plane. Its shape is elongated with a high degree of oblateness, approximating a cigar shape. The central bulge exhibits a bright, concentrated luminosity gradient, suggesting an older stellar population dominating the core. The disk is visible but less prominent, displaying a mottled texture possibly indicative of some star formation, although at a low rate. The overall color profile reveals a redder hue, suggestive of a more evolved stellar population and potentially higher dust content. There is no indication of a major ongoing merger, though some minor disturbances or tidal features might be present. The galaxy exhibits a smooth appearance, though some faint features may be present within the disk.
