The galaxy presents as an elliptical morphology, cigar-shaped with a slight tilt relative to our line of sight. Its light profile appears smooth and centrally concentrated, with a gradual falloff in intensity towards the outer regions. There is no discernible spiral arm structure or prominent dust lanes visible. The central region exhibits a bright, compact core that may host an active galactic nucleus. The colour profile is indicative of a passively evolving stellar population, dominated by older, redder stars. Weak signatures of ongoing star formation are possibly present, seen as blue colourations that seem to be more dispersed in the galaxy. The overall structure suggests a relatively relaxed system, not undergoing major mergers, but minor disturbances are possible given its shape.
