The galaxy appears to be an elliptical type, exhibiting a generally smooth morphology with a high degree of central concentration. The light distribution suggests a dominant spheroidal component. There is no distinct spiral arm structure visible; instead, the light tapers off gradually from the core. The galaxy is moderately elongated, approaching a cigar shape, but mostly in between round and cigar shaped. There is no clear evidence of any major ongoing merger activity or strong tidal disturbances, though a faint asymmetric feature may indicate a minor interaction or internal disturbance. The galaxy presents a yellowish-red hue, indicative of an older stellar population with relatively low levels of current star formation. The overall impression is of a relatively quiescent system transitioning to a passive evolutionary state.
