The galaxy presents a generally smooth, elliptical morphology with a high degree of central concentration. The light profile appears to be dominated by an older stellar population, exhibiting a color gradient that transitions from a redder core to bluer outer regions. The core exhibits a distinct reddish hue, indicative of older, cooler stars and potentially significant dust extinction. The outer regions show a more complex structure, with evidence of fainter, bluer light, possibly associated with more recent star formation activity, although the overall rate of star formation appears relatively low. There is little evidence of spiral arm structure or significant dust lanes. Minor asymmetries may indicate a recent or ongoing minor merger event.
