Observed at a redshift of approximately 0.27, this galaxy appears to be part of a binary system, or in the process of merging with another galaxy. The primary galaxy displays a generally elliptical morphology, exhibiting a cigar-shaped profile. Its light distribution is relatively smooth, suggestive of an older stellar population. The color is notably redder than typical spiral galaxies at similar redshifts, consistent with a low star formation rate and a higher proportion of evolved stars.

The secondary galaxy is smaller and more elongated, potentially a dwarf galaxy undergoing tidal disruption. There is a slight indication of disturbances within the system, implying a degree of interaction between the two galaxies. This interaction could potentially be fueling low-level star formation or triggering morphological changes within the primary galaxy over time. Based on its absolute magnitude, this is a fairly bright galaxy. Further observations would be helpful to understand the dynamics of this system.
