The galaxy appears as a relatively smooth and centrally concentrated object. There is little evidence of significant spiral arm structure or strong irregularities. The light profile appears to fade gradually from the center outwards. It shows some features that could be described as faint disks or more amorphous arms. Its shape appears to be neither perfectly spherical nor highly elongated, placing it somewhere in between. There are no obvious signs of ongoing major mergers or strong tidal disturbances that would suggest a recent interaction.
