The galaxy presents a smooth, elliptical morphology with a high degree of central concentration. There is no discernible spiral structure or prominent dust lanes. The galaxy's shape appears to be slightly elongated, approaching a cigar-like form. Its color is generally yellowish-orange, suggesting an older stellar population and lower rates of ongoing star formation. There is a noticeable color gradient, with the central region appearing brighter and more yellow compared to the outer regions which seem redder. No signs of major mergers or significant tidal disturbances are apparent. The galaxy's overall appearance suggests it is a relatively quiescent system, likely composed primarily of older stars.
