The galaxy appears as a relatively compact and centrally concentrated system. It exhibits a generally smooth morphology, with no obvious spiral arm structures or significant dust lanes visible in this image. The light distribution suggests a centrally dominant bulge component. The overall color profile is relatively uniform, although there appears to be a slight bluer hue in the central region, potentially indicating ongoing star formation. There are no strong indications of any tidal disturbances or interactions with other galaxies.
