The galaxy presents a primarily smooth and elliptical morphology, exhibiting a high degree of central concentration. The overall light distribution is relatively uniform, lacking prominent spiral arm structures or distinct features. The object is moderately bright, suggesting a substantial stellar population. The shape appears somewhat elongated, transitioning between round and cigar-shaped, without sharp definition. There is a slight indication of minor disturbances in the overall structure. The dominant color is a warm, reddish hue, indicative of an older stellar population with lower ongoing star formation. The spatial extent of the galaxy appears compact. There seems to be no significant interaction with nearby galaxies, nor do we see obvious signs of a recent merger event.
