The galaxy presents as a centrally concentrated object with a predominantly smooth morphology. Its overall shape appears somewhat elliptical, elongated in a particular direction, although not severely so. The light distribution is centrally peaked, with a gradual decline in intensity towards the outer regions. The color profile suggests the presence of an older stellar population, dominated by redder hues, with a hint of bluer color. There are some subtle, very small hints of minor disturbances and a few features, indicating ongoing activity or past interactions. This galaxy does not appear to be undergoing a major merger.
