The galaxy presents as an elongated, lenticular structure, exhibiting a smooth, featureless morphology with no distinct spiral arm structures. Its shape is notably cigar-shaped, with a high degree of ellipticity. The galaxy's color profile suggests a relatively quiescent stellar population, with a redder hue indicating older stars and a lower rate of ongoing star formation. There is no obvious indication of any major merging activity or significant tidal disturbances. Minor disturbances may be present, but are difficult to ascertain from the image alone. The galaxy appears to be a relatively isolated object, as there are no interacting companions observed in close proximity.
