The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a central bulge that appears slightly elongated, tending toward a cigar shape. The light distribution suggests a higher concentration of older stars in the core, with colors trending toward the red end of the spectrum, becoming slightly bluer as you move towards the outskirts, indicating some presence of more recent star formation. There is no noticeable evidence of spiral arms or a prominent disk component, suggesting it is not a spiral galaxy. Overall, the galaxy appears to be relatively isolated, without strong signs of ongoing major merger activity or tidal disturbances, although a very faint and small structure appears close to it that may indicate some level of interaction.
