The galaxy presents as a relatively smooth, elliptical morphology with a prominent central bulge. The galaxy's light is concentrated towards the core, indicating a high stellar density in that region. The color gradient suggests that the central region is populated by older stellar populations, exhibiting a yellowish-orange hue. 

There is an extension from the lower portion of the galaxy which also has an orange hue. This may be a tidal tail from a merging event, or a background object. If it is a tidal tail, this implies a history of gravitational interaction, possibly a minor merger. Alternatively, it might be a region of concentrated star formation within the galaxy, though its distinct color and separation suggest otherwise. The galaxy shows no distinct spiral arm structure or prominent dust lanes. Overall, the galaxy appears to be a quiescent system with a lack of significant ongoing star formation outside of the lower orange extension.
