The galaxy presents a generally smooth morphology with a concentrated central bulge. The overall shape appears elliptical, tending towards a slightly elongated, cigar-like form. There is no strong evidence of spiral arm structure. The light distribution is dominated by a yellowish-white hue, suggesting an older stellar population with relatively low ongoing star formation. Subtle color variations in the outer regions may indicate areas of differing stellar populations or dust content. There is a very faint indication of possible tidal disturbances or a minor merging event but this is not conclusive. 
