The galaxy appears to be an interacting system, possibly in the early stages of a merger. The primary galaxy presents a relatively smooth, elliptical morphology with a concentrated central bulge exhibiting a yellowish hue. A secondary, smaller galaxy is visible to the lower left, also displaying a smooth appearance and similar coloration but with a slightly more compact form. There is evidence of tidal disruption or gravitational interaction between the two galaxies, suggesting a dynamic process of merging. The overall system demonstrates intermediate luminosity and an apparent quiescent star formation rate. Further spectral analysis would be required to fully characterize the stellar populations and determine the precise nature of the interaction.
