The galaxy presents as an elliptical morphology, with a high degree of central concentration. The light distribution appears smooth and relatively featureless, indicative of an older stellar population. There is little evidence of spiral arms or a prominent disk structure. The color profile suggests a redder hue, consistent with a population of older, redder stars and a lower rate of ongoing star formation. The overall shape is mostly round. There is no obvious sign of any recent or ongoing major merger activity, with no distinct tidal tails or highly disturbed morphology. Faint asymmetries could indicate a minor interaction, but these are not pronounced.
