The galaxy presents as a relatively compact, spheroidal object. Its central region appears to be dominated by a bright, smoothly distributed light profile, suggesting an older stellar population. The lack of well-defined spiral arms or prominent dust lanes indicates a system with little ongoing star formation. Faint blue hues in the outer regions may suggest some presence of younger stars, but the overall morphology is consistent with that of an elliptical or lenticular galaxy. The smoothness of the light distribution implies a relaxed, dynamically evolved system, potentially nearing the end of its active star-forming phase. There may be signs of a minor tidal disturbance or interaction, although this is not very clear from the images.
