The galaxy presents as a relatively smooth, elliptical form, exhibiting a high degree of central concentration. The light profile appears to decrease radially from the core. Color gradients are subtle, transitioning from a yellowish central region to slightly redder hues in the outer parts of the galaxy. There is no apparent spiral structure, bar, or prominent dust lanes. The overall morphology suggests an early-type galaxy, potentially a spheroid dominated by an older stellar population. There is no indication of ongoing major merger activity or significant tidal disturbances. The galaxy has a moderate size.
