The galaxy presents as a moderately bright object exhibiting an intermediate redshift. It appears to be an interacting system comprised of two dominant components. The primary component is a relatively smooth, centrally condensed object, elongated along a north-south axis. A secondary component, also exhibiting a generally smooth profile, is situated closely to the northeast. There is a faint tidal tail or bridge extending between the two components, suggesting gravitational interaction. Overall, the object displays no strong evidence of spiral arm structure or pronounced star formation regions within its central body. The galaxy's color is indicative of a more evolved stellar population, with a bias towards redder wavelengths. The overall morphology suggests a possible early-stage merger or close interaction between two galaxies, exhibiting characteristics of a system undergoing dynamic evolution.
