The galaxy presents an elongated morphology. The primary component appears to be a bulge-dominated system, exhibiting a smooth, elliptical structure. The luminosity profile suggests a concentrated central region. A secondary, smaller, and more compact component is located in close proximity to the main galaxy, possibly indicating an ongoing or recent interaction. The color gradient shows a generally redder hue, potentially associated with an older stellar population. There may be evidence of tidal disruption or other gravitational disturbances. The galaxy has some star formation, but it is likely not very active at the current redshift.