The galaxy presents as a somewhat elliptical, likely disk-dominated system. Its core region exhibits a high degree of central concentration, appearing bright and slightly yellowish, indicative of an older stellar population. The galaxy displays a relatively smooth overall morphology, suggesting a lack of significant recent major merger events. Some fainter, bluer light extending outwards hints at possible regions of recent star formation in its outer regions. There is a suggestion of minor tidal disturbances or asymmetrical features possibly indicative of an ongoing minor interaction.
