The galaxy presents a generally smooth and somewhat elliptical morphology. There appears to be evidence of an interaction or possible merger event occurring. One galaxy appears to be more centrally concentrated and brighter, while the other is less defined and may be a smaller companion galaxy. The system exhibits a yellowish hue, suggesting an older stellar population with lower star formation rates. The primary galaxy is of intermediate size with no apparent disk features or spiral arm structure visible. The smaller companion galaxy is less well-defined with a bluer tint to the light, possibly indicating ongoing star formation within it.
