The galaxy presents a generally smooth morphology with evidence of internal features. The central region appears bright and relatively concentrated with a yellowish hue. Surrounding this core is a less defined, more diffuse area exhibiting a redder color profile. This suggests potential regions of on-going or recent star formation, or a difference in stellar population age and metallicity compared to the core.

The galaxy exhibits a slightly elliptical shape, appearing close to circular with some deviation. There is also the suggestion of a nearby small object or disturbed feature on one side which may be a result of gravitational interaction, minor disturbance or the tidal effects of a merger.
