The galaxy presents as a somewhat elongated structure, with a noticeable central bulge region exhibiting a yellowish hue, indicative of an older stellar population. Moving outward from the center, there appears to be a faint disk component that is not particularly well defined, appearing relatively smooth in texture. There is some indication of possible disturbances or minor irregularities in the outer regions, although the overall morphology is generally undisturbed. The galaxy is slightly tilted from our line of sight, revealing a somewhat flattened shape. There is evidence of a low level of ongoing star formation, though it does not appear to be particularly active.
