The galaxy presents a moderately concentrated, elliptical morphology. It appears largely featureless, exhibiting a smooth light distribution that decreases in intensity from a bright central core outwards. There is a slight elongation observed, not quite circular but not exceptionally flattened either. The galaxy lacks any obvious spiral arm structure or prominent dust lanes.

The color profile indicates a population of older stars, with a yellowish-red hue in the central regions. Fainter, bluish regions may be present in the outer parts of the disk, suggesting a low level of ongoing star formation, though the overall color suggests a low star formation rate. The overall appearance suggests a mature galaxy that has largely exhausted its gas supply. There is no significant morphological evidence of a recent or ongoing merger, although subtle tidal features cannot be ruled out based on this image alone.
