The galaxy presents as a generally smooth object with a central concentration of light. Its overall shape is elongated, appearing cigar-shaped, though without well-defined spiral arms or a prominent disk structure. The light distribution is not uniform, suggesting varying stellar populations or dust obscuration. A faint blue tinge is observed in the outer regions, possibly indicating ongoing or recent star formation, though the global star formation rate appears relatively low. No signs of significant merger activity, such as tidal tails or distorted morphology, are readily apparent, suggesting it is a relatively isolated system. The central region has a reddish hue.
