The galaxy appears to be a relatively smooth, elliptical type. Its light profile exhibits a concentrated central bulge that gradually fades into a more diffuse halo. The core displays a yellowish hue, suggesting an older stellar population. The outer regions show a slight bluer tint, indicating some presence of younger, hotter stars, though this is not extensive. There are no distinct spiral arms or dust lanes visible, implying a lack of significant ongoing star formation. The galaxy's overall shape is slightly elongated but mostly rounded. There is no visual evidence of any major mergers or tidal disturbances affecting its structure.
