The galaxy presents as an elongated, somewhat cigar-shaped structure, indicative of an elliptical or lenticular morphology. Its light profile appears smooth, lacking prominent spiral arms or distinct features. A concentration of light is visible towards the center, suggesting a bright galactic nucleus. The color gradient transitions from a reddish hue in the core to a bluer tint in the outer regions. There are no readily discernible signs of ongoing major mergers, tidal disturbances or strong irregularities.