The galaxy appears to be an elliptical type, exhibiting a generally smooth morphology with a concentrated central bulge. It shows a subtle elongation but lacks a clear disk structure. A slight disturbance is visible, implying an ongoing or recent interaction, possibly a minor merger event or tidal interaction with another galaxy. The overall color suggests a population dominated by older stars, but with a hint of recent star formation indicated by localized regions of bluer light. This galaxy's reddish hue points to relatively low ongoing star formation rates and a significant population of evolved stars. The central region appears more concentrated and brighter, indicative of a supermassive black hole.
