The galaxy appears as a single, moderately luminous, centrally concentrated object with a smooth profile. Its morphology suggests an elliptical classification, as it lacks discernible spiral arms or a prominent disk structure. The galaxy exhibits a yellowish-orange color, indicating a population of older stars and a relatively low rate of ongoing star formation. The size is relatively compact. There is no clear evidence of significant tidal disturbances or interactions with other galaxies. The high degree of central concentration suggests a significant bulge component. 
