The galaxy appears to be a relatively smooth, elliptical galaxy exhibiting a cigar-like shape. The color profile indicates a redder hue, likely due to an older stellar population or dust obscuration. There is no clear evidence of spiral arms, or disk-like features, suggesting a lack of significant recent star formation. There does not appear to be any ongoing merging activity or major disturbances. The galaxy's light profile is concentrated, consistent with a high degree of central stellar density.
