The galaxy presents as a relatively compact object, exhibiting a smooth, elliptical morphology. It appears elongated, with a cigar-like shape. There is some evidence of minor disturbances in the galaxy's structure. These disturbances could indicate a previous interaction or a minor ongoing merger. The galaxy exhibits a color gradient, appearing bluer towards the central regions. This suggests a higher concentration of younger, hotter stars in the core of the galaxy, with a slight dust lane visible on the left side of the core. Faint extensions of light can be seen emanating from the central region, hinting at a possible tidal tail or other forms of galactic interaction.
