The galaxy presents a largely smooth, elliptical morphology. There is a concentrated central bulge that seems to be devoid of significant dust lanes or spiral arm structures. The color gradient suggests a relatively older stellar population, with the core exhibiting a yellowish to reddish hue, indicative of evolved stars. There is little evidence of ongoing star formation. The general shape of the galaxy is close to circular, with a slight elongation. No signs of recent major mergers or tidal disturbances are easily observed in this image. The object appears as an isolated galaxy, with no immediate companions or indications of strong gravitational interaction.