The galaxy presents a generally smooth and rounded morphology, with a dominant central bulge exhibiting a bright, yellowish hue, suggesting an older stellar population. There is limited evidence of distinct spiral arms or a well-defined disk structure; rather, the galaxy appears more spheroidal in nature. Faint, bluer regions are observed in the outer regions, possibly indicative of ongoing, albeit subdued, star formation. The overall light distribution is centrally concentrated, decreasing in intensity towards the edges. There is little evidence of major mergers or significant tidal disturbances, suggesting a relatively quiescent evolutionary history. The galaxy exhibits colors that span from blue to yellow, though the exact distribution of color is difficult to define.
