The galaxy presents a largely smooth morphology, with a high degree of central concentration. The color profile is dominated by redder wavelengths, indicative of an older stellar population. The overall shape is elliptical, tending towards a slightly elongated spheroid. There is no clear evidence of spiral arms or significant dust lanes. Subtle disturbances may be present, though the resolution is not adequate to definitively identify any merging activity or tidal features. Based on the color and smooth appearance, this galaxy may be a relatively massive, early-type system with suppressed star formation.
